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Science / Space Race

[July 22, 1967] Getting the mail through (Australia introduces Postcodes)

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by Kaye Dee

In my first article for the Journey, just over three years ago, I talked about rocket mail and flying postmen. Well, we haven’t seen either of them yet – despite continual promises that they are “only a few years away”. This month, though, Australia has taken a step into the future of postal technology with the introduction of Postcode, the new national mail sorting system.

Zipping the Mail Along
Postal codes are not exactly new. They were first developed in large cities like London (where they were introduced in 1857) to help improve the speed of mail sorting and delivery as populations and the size and complexity of cities grew.

Modern postal codes were first introduced in the Ukrainian Soviet Socialist Republic in 1932, followed by Germany (1941), Singapore (1950) and Argentina in 1958. Britain began introducing its current postal code system in 1959, while the US Postal Service introduced the five-digit ZIP code in 1963. I was interested to learn as I prepared to write this article that the ZIP part of ZIP code is actually an acronym standing for Zone Improvement Plan. I always thought that it was just a play on the idea of zipping, or speeding, the mail along to its destination. Switzerland was the most recent country to introduce postal codes before Australia, in 1964.

Mechanising Mail Sorting
What made the Postmaster General’s Department (PMG), which manages all Australia’s postal, telephone and telegraph services, decide that we needed to follow suit and speed up our mail by using a postal code system? After all, Australia’s current population is only 11.87 million – less than the population of New York City, which I understand is about 15.6 million.

Until now, mail sorting in this country has primarily been done by skilled human sorters, who have a detailed knowledge of geographical localities, reading the address on each letter. However, there are about 8,000 delivery offices around the country, so getting the mail to its final destnations has required at least two or three stages of sorting.


Mail sorting at the Sydney General Post Office in 1964

Australia has long been a world leader in in postal service mechanisation, and as early as 1958, the PMG decided to introduce large-scale mechanical mail sorting systems across Australia. As the first stage of this plan, the Sydney Mail Exchange opened in the suburb of Redfern in 1965, to automate and centralise the mail sorting facilities for New South Wales. It’s the largest and most advanced mechanised mail centre in the Southern Hemisphere, and the new electronic equipment and technology is attracting Worldwide interest. I’ve even heard that the Mail Exchange’s design concept is being considered as a possible future system by the US Postal Service.


Sydey's ultra-modern new mail exchange, in the inner-city suburb of Redfern

Sydney is our largest city, and New South Wales, the most populous state, so it makes sense to introduce a new Postcode system to work in conjunction with the state-of-the-art electronic mail handling equipment at the Sydney Mail Exchange, through which so much mail passes. Postcodes simplify the sorting process, as the mail sorter is now a coding operator, who enters the postcode using their data entry terminal, enabling the letters to be rapidly sorted electronically and speedily despatched to their delivery offices.


The Sydney Mail Exchange's state-of-the-art data entry system for the new sorting computers. Conveyors drop individual letters in front of the operators, who then type the postcode or suburb identifying the letter’s destination

The computers controlling this process occupy a large amount of space in the Mail Exchange building. Similar mechanised sorting systems will be gradually introduced around the country over the coming years: they’ll be immediately able to take advantage of the Postcode system to speed their mail sorting, without many of the teething problems that have bedevilled the Sydney mail Exchange.

The Australian Postcode System
The Postcode system was introduced on Saturday, 1 July. The new four-digit number system replaces some earlier postal sorting systems, such as Melbourne's letter and number codes (e.g., N3, E5) and a similar system that has been in use in rural and regional New South Wales. Nearly 5,000 postcodes have been allocated across the country, to every city, town, suburb and small regional centre.

Postcodes have been allocated following a broad geographical pattern, with Postcode numbers for capital city suburbs beginning in the west and moving to the north, east and south. A similar pattern is followed for regional country areas. The first digit of the Postcodes in each station corresponds to radio station call signs for that state: 2 (New South Wales and the Australian Capital Territory – our equivalent of the District of Columbia), 3 (Victoria), 4 (Queensland), 5 (South Australia), 6 (Western Australia), 7 (Tasmania) and 8 (Northern Territory).

I think this is a good idea because everyone knows the radio callsigns, so it will make it easier to remember Postcodes for their friends locally or interstate. Subscriber Trunk Dialing for telephones, which commenced last year, is also using the state radio call sign number as the basis of the dialing codes for each capital city, so I imagine that will help with remembering the direct dial codes too. 

Getting the Word Out

The first edition of the Postcode booklet, listing every national Postcode, is being distributed free by mail this month to every Australian household and business address. A total of 4.5 million booklets are expected to be distributed, along with a postcard identifying the recipient’s own postcode. Of course, with 5,000 postcodes to include in the booklet, and with some geographical oddities to contend with, it’s not surprising that diligent nit-pickers have already found faults in the booklet to complain about and have been writing carping letters to the editors of local and major state newspapers.

There has been extensive advertising about the new Postcode system in the newspapers and on television and radio, but so far, we have not been treated to a catchy jingle like the one that introduced us to decimal currency last year.

The PMG is hoping that if we all start using the Postcodes properly at the end of addresses, not only will it improve the speed of mail delivery, but that next year it will make it easier to introduce “post office preferred-size envelopes” as well, whose standardised sizes will further improve the speed of mechanised mail sorting! 

And then I can finally get my postcards from the Traveler in a timely manner!



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Science / Space Race

[June 28, 1967] Around the World in Two Seconds (Our World Global Satellite Broadcast)

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by Kaye Dee

I love how our world is drawing closer every day to some of the amazing futures that science fiction has spread before us. I’ve written before about the importance of satellite communications in connecting this divided planet. Just two days ago, 24 countries around the globe were linked together in the first world-spanning live satellite broadcast, titled – appropriately enough – Our World.

Our World's visual symbol incorporates a modernised version of da Vinci's "Vitruvian Man", with arms encircling the globe, and vertical and horizontal lines representing longitude and latitude

Continue reading [June 28, 1967] Around the World in Two Seconds (Our World Global Satellite Broadcast) →

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Science / Space Race

[June 14, 1967] What's Easy for Two (Venus 4 and Mariner 5)

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by Gideon Marcus

Red Venus?

Every 19 months, Venus and Earth reach positions in their trips around the Sun such that travel to the former from the latter uses a minimum of energy. Essentially, a rocket blasts off and thrusts itself toward the Sun just long enough to drift inward and meet Venus after about half an orbit (a direct path would be very costly in terms of fuel use). The less energy used, the bigger the spacecraft can be sent. That means more payload for experiments.

The Soviets have been trying to reach the Planet of Love, Earth's closest neighbor (besides the Moon) for more than six years now. In February 1961, they launched Venera 1 (Venus 1), the first interplanetary probe to fly by another world–but it had gone silent by the time it got there.  Veneras 2 and 3 went up three opportunities later, in November 1965, but fell silent the next spring, just before reaching their target.  Indeed, Venera 3, a soft-lander, is believed to have rammed the cloud-shrouded world, becoming the first artificial object to reach another world.  Either way, no useful data was received.

Why didn't they launch any Veneras in 1962 or 1964?  In fact, it looks like they did.  The Soviets don't herald their failures.  Nevertheless, according to NASA officials, we have a pretty good catalog of them, thanks to careful parsing of Russian news reports as well as radar and telemetry data we've managed to gather.  Three Russkie Venus probes were launched in September 1962 and three more in February 1964.  Getting out of Earth orbit can be tough, requiring a second firing of onboard engines once a spacecraft is circling our planet.  Apparently, these six probes never got away.

But Venera 4, launched on June 12, 1967, has apparently passed that first hurdle.  Moreover, at one and a quarter tons, it is several hundred pounds heavier than any of its predecessors.  We don't know much about what's on the latest Communist probe, but scientists speculate some of the extra weight has been devoted to heat shielding.  Venus is very hot, perhaps 900° Fahrenheit, and it is believed that heat is what caused Venera 3 to fail.  Given that TASS, the Soviet news service, reported that Venera 4 is going to Venus, rather than by, it is assumed the spacecraft will make another landing attempt.

Provided it doesn't go slient like its predecessors.  Communicating across planetary distances is a hurdle the Soviets only recently surmounted with their Zond 3 probe, which tested radio reception at about 150 million kilometers' distance–far enough for a Martian mission.  Essentially, Zond 3 was the Soviet version of Pioneer 5–but five years later.  This is suggestive as to the Soviet level of communications technology, at least.  America would seem to have the clear lead there.

Well, I wish the Soviets luck.  Politics or no, I want to know more about that mysterious, seared world that is Venus!

Yankee Two-dle

If Venera 4 fails, it has a back-up of sorts.  Mariner 5, itself a back-up for the Mars-bound Mariner 4, was launched today early this morning, destination: Venus.

Already several hundred thousand kilometers from Earth, zooming at more than 10,000 kilometers per hour, it should reach Venus in October.  The spacecraft, launched via Atlas-Agena, the same rocket that launched our first Venus probe, Mariner 2, is barely a quarter the mass of Venera 4.  Moreover, Mariner 4's TV camera has been deleted, a decision that likely irks Venus scientist Dr. Carl Sagan, who insists doing so is short-sighted, clouds or no. 

But that removal, along with the reduction in the size of the solar panels (less is needed so close to the sun) means that when Mariner 5's planned flight path brings it within 3000 kilometers of Venus, it will be able to investigate the planet with a wide suite of instruments.  An ultraviolet photometer should not only refine temperature estimates of the Venusian upper atmosphere, it will tell us a bit about what gasses constitute it.  For instance, if there be any water there, perhaps life exists in the cloud tops, above the intense heat at the surface.

The rest of the instruments are likely ho-hum for the general audience, but should return a bonanza for scientists.  They include a magnetometer and various radiation sensing equipment that not only will measure the Venusian version of the Van Allen Belts (if they exist–Mariner 2 couldn't find any), but also tell us a lot about the solar wind on the way to Venus.

I will say, I'm glad we're sending a craft to Venus, and it does seem we did it on the cheap ($35 million), but I think I'm with Sagan on this one: for all the effort, it seems we're not going to find out very much about Venus with Mariner 5.  Another reason to root for Venera 4.

And a good reason to write your Congressman about the importance of planning a bigger Venus shot, perhaps on the more powerful Atlas Centaur rocket, when the next opportunity rolls around in January 1969!

Want to find out what we currently know about Venus?  Come read our previous articles on the planet of love!



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Science / Space Race

[May 28, 1967] Around the World in 80 Months (May 1967 Space Roundup)

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by Gideon Marcus

Between the tragic aftermath of this year's twin space disasters (Apollo 1 and Soyuz 1) as well as the dramatic results from the Lunar Orbiter and Surveyor Moon explorers, it's easy to forget the amazing things being done in Earth orbit.

So here's a little news grab bag of some flights you may have missed over the last several months (and even years, in some cases):

Moscow calling

Two years ago, the Soviets joined the world of comsats with the orbiting of their first Molniya satellite.  Launched into an eccentric orbit that takes them up to geosynchronous altitudes but then swooping down to graze the Earth, they work in pairs to facilitate transmissions across the 11 time zones of the Soviet Union.

It's an impressive system–half a ton of satellite broadcasting at 40w of power, more than twice that of the Intelsat "Early Bird" satellites.  Unfortunately for the Soviets, it's also been a balky system.  Both of the first two satellites stopped working within a year, Molniya 1B failing to keep station in space.  It's a bad thing when your comsat moves out of position!  This is something more likely to happen in an eccentric orbit than in a more-stable geosynchronous orbit where a satellite goes around the Earth once every 24 hours, remaining more or less stationary (except for a little figure eight over the course of the day) from the perspective of the ground observer.  Worse, because the Molniyas scrape so close to the Earth, it doesn't take much to send them careening into the atmosphere, which happened to 1B March 17, 1967.

Still, the Soviets prefer their odd orbit because it's ideal for their purposes (giving coverage to Eurasia) and, I suspect, requires less booster power.  And it still carries the satellites high enough to return photos like this one, shot by Molniya 1A last year–the first all-Earth photo ever:

Molniya 1C was launched on April 25 last year, Molniya 1D on October 20.  They were replacements for their non-functioning companions.  But Molniya 1C may well have given up the ghost, too.  Molniya 1E was launched on May 24, apparently to replace it. 

May they solve their teething problems sooner rather than later!

A Pair of Imps

Out beyond the Earth's magnetic field is the sun's domain.  High energy plasmas (the "solar wind") and our star's magnetic field fill the vacuum of interplanetary space.  Not very densely, to be sure, but with profound effects on the planets and offering clues as to the nature of the stellar furnace that creates them.

It is not surprising that NASA has devoted so many satellites to understanding and mapping this zone given how many spacecraft (including the upcoming Apollos) will travel through it.  Explorer 18, Explorer 21, and Explorer 28 were all part of the "Interplanetary Monitoring Program" (IMP).  The first two have already reentered, and the last just stopped working a couple of weeks ago.  Luckily, virtually uninterrupted service has been maintained thanks to the launches of Explorer 33 and Explorer 34!


Explorer 33

Explorer 33, launched July 1, 1966, was supposed to be the first of the "anchored" IMPs, returning data from the orbit of the Moon (which does not have a magnetic field or radiations of its own).  Unfortunately, the satellite was shot into space a bit too rapidly to safely decelerate into orbit around the Moon.  Instead, it now has an extremely high (270,000 miles perigee!) but eccentric (low apogee) orbit from which it still can return perfectly good science.  Indeed, NASA planned for this eventuality.


Explorer 34

The other Explorer, #34, was just sent up on May 24.  It is a more conventional IMP and will pick up where #28 left off. 

With four years of continuous data, we now have terrific data sets on the Sun through a good portion of its 11-year cycle, including the recent solar minimum.  I look forward to a slew of reports in the Astrophysical Journal over the next few years!

Yes, I read those for fun.  Doesn't everyone?

Bright Future

If the IMPs exist to monitor the Sun's output, the Orbiting Solar Observatories' job is to directly watch the Sun.  Prior to 1967, two of these giant satellites had been orbited: OSO 1 on March 7, 1962, and February 3, 1965.  A third launch was made on August 25 of the same year, but it failed.

Sadly, the OSOs haven't quite provided continuous coverage over the last five years.  Still they have returned the most comprehensive data set of solar measurements to date.  And, as of March 8, the wiggly needles that mark the collection of data are jiggling again: OSO 3 has been returning data from its nine instruments on all manner of solar radiation–including and especially in the ultraviolet, X-Ray, and cosmic ray wavelengths that are blocked from terrestrial measurement by the Earth's atmosphere.

The timing is perfect–the Sun is just entering its period of maximum output.  OSO 3 will not only tell us more about the nearest star, it will report on its interactions with the Earth's magnetic field and the space environment in near orbit.

A Meteoric Rise

The Soviets have been awfully cagey about a lot of their launches.  Every couple of weeks, another unheralded Kosmos heads into orbit, stays there for a week, then lands.  It's an open secret that they are really Vostok-derived spy satellites that snap shots and return to Earth for film development.  This is utterly reprehensible–certainly WE would never do anything like that.

But while many of Communist flights have been hush hush, one subset of their Kosmos series has been pretty open: the weather satellite flights of Kosmoses 122, 144, 149, and 156!

The first of the Soviet meteorological satellites went into space on June 25, 1966, broadcasting for about four months before falling silent.  For a while, it seemed the Russkies were going to keep the pretty weather photos to themselves, but on August 18 of last year, they suddenly started sharing data over the Washingon/Moscow "Cold Line"–both visibile and infrared pictures, too.  It appears the delay was due to the Soviet reluctance to announce a mission until they're sure of its success.  It is entirely possible that some of the unexplained Kosmoses before 122 were failed flights.


Kosmos 122

The picture quality was pretty low at first, probably due to the length of the line the data must be sent over.  Improvements were made, and the new stuff is great.

Since 122, the Soviets have launched Kosmos 144 on February 28, 1967, Kosmos 149 on March 21 (it reentered on April 7–a failure of its weather-related mission, but it successfully tested the first aerodynamic stabilizer in orbit), and the latest Kosmos, #156, just went up on April 27, 1967.  It is my understanding that photos are being regularly shared with the National Environmental Satellite Service (NESS) in Suitland, Maryland.  I don't know if these are revolutionizing our view of the planet given our successful ESSA and NIMBUS programs, but it does give a warm glow of international cooperation.

If the nukes fly, at least we'll know if it's nice weather over their targets…

From the Far East into the Drink

The Japanese have been working their darndest to become the sixth space power (after the USSR, US, UK, France, and Italy).  Unfortunately, all of their efforts have thus far come up a cropper.

Their Lambda 4S rocket is the first one capable of launching a satellite into orbit, specifically an ionospheric probe with a 52 pound science package.  The problem is the vehicle's fourth stage.  The truck-launched Lambda 3 has been pretty much perfected, but when the new engine was put at the top of the stack, everything went to hell.


The successful precursor of the Lambda 4S, the Lambda 3

On September 26, 1966, the first Lambda 4S was lost when the fourth stage attitude control failed.  The fourth stage didn't even ignite the second time around on December 20.  That happened again on April 13 of this year during the third flight.

It looks like Nissan and JAXA engineers will be going back to the drawing board before trying another flight.  Maybe 1968 will be the year the Rising Sun joins the rising sun above the Earth…

What's next?

This summer, our eyes will surely turn beyond the Earth to Earth's twin, the planet Venus, for June marks the latest opportunity to send probes to the second planet at a premium on fuel consumption and payload allowance.  You can bet we'll be covering Mariner 5 and Venera 4 when they launch!


Testing Mariner 5



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Science / Space Race

[January 28, 1967] "Fire in the cockpit!" (The AS-204 Accident)

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by Kaye Dee

As I write this, I’m still in shock. It’s only a few hours since the news broke here in Australia of the tragic loss of the crew of Apollo 204 in a fire on the launchpad at Cape Kennedy, during a launch rehearsal. Spaceflight is difficult and dangerous – we know that. Astronauts Freeman, Bassett and See were killed in plane crashes during training; Armstrong and Scott had a narrow escape from inflight disaster during Gemini VIII.

Unconfirmed rumours abound of Soviet cosmonauts who died in unsuccessful space missions before Gagarin, and the Russians have probably had training accidents to which they have not yet admitted. When I wrote about Gemini VIII’s aborted mission, I asked if spaceflight was moving too fast. There’s certainly been a headlong rush on NASA’s part to get to the Moon ahead of the Soviet Union, so perhaps this tragedy is the answer to my rhetorical question.


The first image available showing the fire-ravaged interior of the Apollo 204 spacecraft

Details are still sketchy at this time, although no doubt more information about the accident will emerge in the coming days and weeks as investigations take place. But right now, let’s explore the background to the mission and what we know about the catastrophe.

The Lost Crew
Apollo 204 (AS-204) was intended to be the first manned test flight of the new Apollo Command and Service Modules, the spacecraft that will be used to carry the first NASA astronauts to the Moon within the next few years. As such, two experienced astronaut test pilots were assigned to the flight: USAF Lt. Colonels Virgil “Gus” Grissom, the Command Pilot, and Senior Pilot Edward White. Grissom was the United States’ second space traveller, flying the Mercury MR-4 mission. He also commanded the first manned Gemini mission, Gemini III. Rumour even has it that Grissom was already under possible consideration to command NASA’s first lunar landing mission. Lt. Col. White is famous as the first American to make a spacewalk, during Gemini IV. These veteran astronauts were joined for this mission by rookie US Navy Lt. Commander Roger Chaffee. Chaffee was selected as a member of the third astronaut group and specialised in communications: he had been a CapCom for both Gemini III and IV.


Official Apollo 204 crew portrait, including a model of the new Apollo Command Module which their mission was intended to test. Left to right Ed White, "Gus" Grissom and Roger Chaffee

The Apollo 204 back-up crew consists of experienced Mercury and Gemini astronaut Walter Schirra and first-time fliers Donn Eisele and Walter Cunningham. Astronaut Eisele had originally been assigned in Lt. Commander Chaffee’s role for the Apollo 204 mission but had to be replaced when he needed shoulder surgery in early 1966. I assume that once Apollo missions resume after the accident investigation, this crew will fly the first orbital mission that should have been accomplished by AS-204.

What’s in a Name?
The design for the official Apollo 204 patch, developed by the crew and illustrated by North American Rockwell artist Allen Stevens, carries the designation Apollo 1. At the time that it was approved by NASA, in June 1966, this was the flight’s official name. However, it seems that only recently some doubt arose as to whether the formal designation of the mission would be Apollo 1 after all, which is why it is presently being referred to as Apollo 204, or AS-204. I’ve heard from the Australian liaison officer at NASA, that just last week approval for the patch was withdrawn and that, if this accident had not occurred, the patch might have had to be redesigned, depending on the final mission designation.

But as it stands, the mission patch uses the American flag for a background, with a central image depicting an Apollo spacecraft in Earth orbit. The Moon appears to the right of the Earth, reminding us of the eventual goal of Project Apollo. The designation Apollo 1 and the names of the crew appear in a border around the central image, while the patch is edged with a black border – a touch that is poignantly even more appropriate in view of the loss of the crew. I do hope that this patch, and the designation Apollo 1, will be re-instated as the official insignia of this mission in honour of its lost crew.

The Mission that Should Have Been
The fire that has killed the Apollo 204 crew occurred during a preflight test ahead of a launch scheduled for 21 February. It was planned to be the first manned orbital test flight of the Apollo Command and Service Modules, launched on a Saturn IB rocket. The mission was to have tested launch operations, ground tracking and control facilities, as well as the performance of the Apollo-Saturn launch vehicle. Depending on how well the spacecraft performed, the mission might have lasted up to two weeks, perhaps equalling Gemini VII's record spaceflight and demonstrating that the Apollo spacecraft could function successfully for the duration of the longest Moon flights currently in planning.


The Apollo 204 crew in front of Pad 34, from which they should have launched, and where they have been killed

The Command Module allocated to Apollo 204, CM-012, was a so-called “Block I” version, originally designed before the lunar orbit rendezvous landing strategy was selected. Block 1 spacecraft aren’t able to dock with a lunar module, but future “Block II” versions will.

Was It a Lemon?
The Apollo Command and Service Modules are undoubtedly far more complex than any previously-built spacecraft, so it isn’t surprising that their development has had many teething problems. Over the last few months, I’ve heard from my former colleagues at the WRE that many issues with the Command Module became evident last year, especially when CM-012 was delivered to Kennedy Space Centre in August to be prepared for its flight. Even before it arrived, the Apollo 1 crew had expressed concerns to Apollo Spacecraft Program Office manager Joseph Shea about the quantity of flammable materials, such as nylon netting and Velcro, being used in the spacecraft cabin to hold tools and equipment in place. It seems that, even though Shea ordered these flammable materials removed, this may not have happened.


The Apollo 204 crew sent Program manager Jospeh Shea a parody of their crew portrait to express their concernes about the spacecraft. They are shown praying, and the picture carried the inscription: "It isn't that we don't trust you, Joe, but this time we've decided to go over your head"  

When CM-012 arrived at Kennedy Space Center, there were still 113 significant planned engineering changes to be completed, and another 623 engineering change orders were made following delivery! This suggests that many issues with the spacecraft design were still being resolved. Apparently, the engineers in charge of the spacecraft training simulators just couldn’t keep up with all these changes, and I’ve heard that Lt. Colonel Grissom expressed his frustration about this by bringing a lemon from a tree at his home and hanging it on the simulator.


CM-012, at that time designated Apollo 1, arriving at Kennedy Space Centre

There were several problems with the environmental control unit in the Command Module, which was twice returned to the manufacturer for designed changes and repairs. During a high-speed landing test, when the Command Module was dropped into a water tank to simulate splashdown, its heat shield split wide open, and the ship sank like a stone! There were also apparently concerns about a propellant tank in the Service Module that had ruptured during pre-delivery testing. NASA had it removed and tested at Kennedy Space Centre to be sure there were no further problems. 

CM-012 finally completed a successful altitude chamber test on 30 December and was mated to its Saturn IB launch vehicle on Pad 34 at Cape Kennedy on 6 January. So, was this particular spacecraft a lemon – an accident waiting to happen? Or has this tragedy shown that the design of the Apollo Command Module is inherently flawed? We’ll undoubtedly have to wait for the results of the accident investigation before we know the answer.

Countdown to Disaster
At this point, we still know very little about the disastrous fire or what led to its breakout, but my WRE colleagues have helped me put together some information accident from their contacts at NASA. The fire broke out during what had apparently been a trouble-plagued launch simulation known as a "plugs-out" test. This kind pre-flight simulation is intended to demonstrate that the spacecraft will operate as it should on internal power, detached from all cables and umbilicals, and successfully carrying out this test was essential for confirming the 21 February launch date.


The AS-204 crew in the CM simulator on 19 January, as part of their preparations ahead of the "plugs out" test

Almost as soon as the astronauts entered the Command Module, there were problems when Grissom experienced a strange odour in his oxygen supply from the spacecraft, which delayed the start of the test. Problems with a high oxygen flow indication that kept triggering the master alarm also caused delays. There were also serious communications issues: at first, it was Command Pilot Grissom experiencing difficulty speaking with the control room, but the problems spread to include communications between the operations and checkout building and the blockhouse at complex 34, forcing another hold in the simulated countdown.

Fire Erupts
It was not until five and a half hours after the simulation began that the countdown finally resumed, and when it did instruments apparently showed an unexplained rise in the oxygen flow into the crew’s spacesuits. Within seconds, there were calls from the spacecraft indicating that a fire had broken out in the cabin and that the astronauts were facing a serious emergency, trying to escape. The final transmission from inside the spacecraft ended with a cry of pain.

Of course, there are emergency escape procedures for the Command Module, but with the triple spacecraft hatch, it requires at least 90 seconds to get it open, and it seems that the crew had never been able to accomplish the escape routine in that minimum time. There is some evidence that Lt. Col. White was trying to carry out his assigned emergency task of opening the hatch, but in the pure oxygen atmosphere of the spacecraft, the fire became incredibly intense very rapidly and rising internal pressure would have made it difficult, if not impossible to open the inward-opening hatch.


Picture taken shortly after the fire was extinguished showing the external damage to the Command Module caused by the hull rupture resulting from the fire

In less than 20 seconds from the first detection of the fire, the pressure inside CM-012 rose to the point where it actually ruptured the hull of the spacecraft, sending flame, heat and dense smoke into the pad service structure. The ground crew bravely tried to rescue the astronauts, but the dangerous conditions and unsuitable emergency equipment made it virtually impossible. Many were later treated for smoke inhalation. There were fears the CM had exploded, and that the fire might ignite the solid fuel rocket in the launch escape tower above it. If this happened, it could set fire to the entire service structure.

It took about five minutes for the ground crew to finally get the spacecraft hatch open, but their efforts were in vain, as the astronauts were already dead. The exact cause of death has yet to be determined: it may have been physical burns from the fire, or carbon monoxide asphyxia, from the fire's by-products.

Whatever the cause, three brave men have died, and an exhaustive investigation of the fire and its causes will now take place as part of the accident investigation. Exactly what effect this tragedy will have on the future of the Apollo programme will very much depend upon the findings of that investigation. If the design of the Command Module is found to be intrinsically flawed, the necessary redesigns could delay the programme for years, causing NASA to miss President Kennedy’s deadline for a Moon landing, and allowing the Soviet Union to overtake the United States again in the Space Race.

Grissom and White have both said in past interviews that they recognized the possibility that there could be catastrophic failures and accidents in spaceflight and that they accepted that possibility and continued with their work. I’d just like to give the last word in this article to Astronaut Frank Borman, who said in a 1965 interview "I hope that the people in the US are mature enough that when we do lose our first crews they accept this as part of the business". It would not honour the loss of the Apollo 204 crew if this tragedy led to the termination of the Apollo programme.



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Science / Space Race

[November 16, 1966] A Grand Finale (Gemini 12)

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by Kaye Dee

As I write, it’s less than a day since the splashdown of Gemini 12 brought NASA’s second manned spaceflight programme to an overwhelmingly successful conclusion, demonstrating that the Space Agency has finally mastered the art of spacewalking. It’s incredible to think that it’s only been 20 months since the first manned Gemini mission was launched, but the packed schedule of ten flights has tested out all the techniques that the space agency needs to advance to its Apollo lunar programme.

Two for the Show

Gemini 12's Command Pilot was former Naval aviator Captain Jim Lovell (left in photo above). Making his second spaceflight, Lovell previously flew on the Gemini 7 long duration mission and now holds the record for the longest time spent in space by any astronaut or cosmonaut. Pilot for this mission was rookie astronaut USAF Major Edwin “Buzz” Aldrin, who performed an unprecedented three successful extravehicular activities (EVAs) during this flight. The only member of the astronaut corps to hold a Doctorate, Aldrin is a specialist in rendezvous and docking techniques, and on this mission he put that knowledge to very good use.

A “Halloween” Patch

Gemini 12 was originally scheduled to launch on October 31, so Lovell and Aldrin had considered a Halloween theme for their mission patch. They wanted to evoke Halloween with the use of orange and black colours and also planned to show their Gemini capsule launched on a witch’s broomstick instead of a rocket! However, with the launch rescheduled to November, only the Halloween colour-scheme remained of the original concept.

The final design features the Roman numeral XII at the top of the round patch, in the position it would be on a clock-face. Just like an hour hand, the Gemini spacecraft points to the XII, a reminder that this is the final flight of the Gemini programme. The crescent Moon on the left side of the patch symbolises the ultimate goal of the upcoming Apollo programme.

Training for Weightlessness

Gemini 12's main goal was to complete three EVAs that would demonstrate that NASA had finally cracked the problem of successfully carrying out spacewalking operations, a technique crucial to the Apollo programme.

The astronauts who attempted to perform spacewalks on Gemini 9, 10 and 11, had all reported that operating in orbit was much more difficult and tiring than the simulations conducted using the KC-135 weightlessness training aircraft. They also complained that there were few handholds on the exterior of the Gemini and Agena to help them move around in Zero-G. Consequently, a new approach to training was employed for Gemini 12, which I understand was suggested by Astronaut Aldrin himself, who is a keen scuba diver.


"Buzz" Aldrin practices installing a handrail between the Gemini capsule and Agena target vehicle, in an underwater training simulation

In addition to the KC-135 flights, Aldrin trained in a large pool containing a Gemini mockup. In the pool, special weights were added to the astronaut’s spacesuit to create “neutral buoyancy,” offsetting gravity so he would neither rise nor sink, and Aldrin spent several EVA simulation training sessions of more than two hours underwater.

As well as this new training technique, more handrails and handholds were added to the Gemini capsule, along with a waist tether that would enable Aldrin to turn wrenches and retrieve experiment packages without too much effort.

Dr. Rendezvous Saves the Day, Again!

After two delays caused by technical issues, the final Gemini mission lifted off on the afternoon of November 11 US time. On its third orbit, Gemini 12 prepared to dock with the Agena target vehicle, but problems with the Gemini's onboard radar threatened to make that impossible.

Luckily, Aldrin had already developed procedures for onboard backup rendezvous techniques in the event of radar failure. Drawing on his expertise, Aldrin used a sextant and his slide rule, measuring the angle between the horizon and the Agena. Once he had confirmed the information with his rendezvous chart, Aldrin calculated corrections with the spacecraft’s computer, enabling the rendezvous and docking to be successfully accomplished.

Rendezvous with the Sun

Despite the successful rendezvous, some anomalies with the Agena’s turbopump during launch led to Mission Control cancelling a planned boost to a higher orbit, like that conducted on Gemini 11. Instead, NASA took the opportunity to have the crew photograph a solar eclipse through the spacecraft windows at the beginning of mission day two.

Using the Agena’s secondary propulsion system, Gemini 12 changed orbits to place itself above South America at the right time and location to capture the first colour images of a total solar eclipse free from the interference of the Earth’s atmosphere. During the scant eight seconds that the astronauts could view the eclipse, they snapped four images that are expected to help scientists discover the secrets of the solar corona. The pictures were taken with film sensitive to ultra-violet light, which does not penetrate through the Earth's atmosphere.

Standing Up in Space

About two hours after photographing the eclipse, Aldrin commenced his first EVA, with his head and upper body exposed to space as he stood in the open hatch above his spacecraft seat. During this “stand-up EVA”, which lasted almost two and a half hours, Aldrin took the time to accustom himself to the space environment, which it was thought would better prepare him for his later spacewalk.

One of his first jobs was to install a handrail between his hatch and the docking collar of the Agena that would aid his movements during his day three spacewalk. Aldrin mounted a camera on the side of the spacecraft, with which he took a close-up picture of himself (above), the first shot of its type ever taken! He collected a micrometeorite experiment, and took photographs of the Earth as well as ultra-violet astronomical photography.

Aldrin’s photographic tasks were part of the 14 scientific, medical, and technological experiments planned for Gemini 12. Although five experiments could not be fully completed, those that were included: frog egg growth under zero-g conditions; synoptic terrain and weather photography; airglow horizon photography; and UV astronomy and dim sky photography.

Walking and Working in Space

Gemini 12 flight day three began with some minor fuel cell and manoeuvring thruster issues that would last for the rest of the mission. They did not, however, prevent the highlight of the flight from taking place: a planned two hour tethered spacewalk by Major Aldrin. Until Gemini 12, successfully performing work outside a spacecraft was the one Gemini objective that had eluded NASA, but Aldrin exceeded even the most optimistic hopes for this flight as he performed a record two hours, nine minute and 25 second EVA.

Attached to a 30-foot umbilical cord, Aldrin used the handrail he had installed the day before to assist in attaching a 100-foot long tether between the nose of the Gemini and the Agena. With the handholds, he did not experience the problems Gordon encountered on Gemini 11. Aldrin’s approach to his spacewalk was to go slowly and carefully, resting for two-minute periods between tasks. In fact, about a dozen two-minute rest periods were built into the EVA schedule to prevent Aldrin from becoming exhausted like previous Gemini spacewalkers. 

Moving to the spacecraft’s aft adapter, Aldrin supported himself with overshoe restraints and waist tethers to carry out a number of work tasks. He was able to fasten rings and hooks, connect and disconnect electrical and fluid connections, tighten bolts and cut cables. Aldrin then moved across to the Agena, where he worked at pulling apart electrical connectors and putting them together again. He also tried out a torque wrench designed for the Apollo programme.

At the completion of his spacewalk, Aldrin returned to his Gemini seat with no fatigue and all his tasks accomplished. This demonstrated that the use of neutral buoyancy training, available handholds and foot restraints on the spacecraft, and a slow and measured pace of work while in space, are the ingredients needed for future successful EVAs during the Apollo missions. 

Going for a Spin

The other major task for flight day three was a repeat of the gravity-gradient stabilisation/artificial gravity experiment performed on Gemini 11. Undocking from the Agena, Gemini 12 moved to the end of the tether connecting the two vehicles and then fired its thrusters to slowly rotate the combined spacecraft. Although they had some difficulty keeping the tether taut, the astronauts were able to use centrifugal force to generate a small amount of gravity during the four hour, 20 minute exercise, and achieve gravity-gradient stabilization. After releasing the tether connected to the Agena, Gemini 12 pulled away from the target vehicle and did not re-dock with it again.

One More Time

The last day of Gemini 12’s mission began with an attempt to sight two yellow clouds of sodium particles ejected by a pair of French Centaure rockets launched from the Algerian Sahara. This experiment was designed to measure high altitude winds. Although Lovell and Aldrin could not see the clouds, they did attempt to photograph them using directional instructions from the ground. We’ll have to wait until those films are developed to see if they were successful.

Shortly afterwards, as the spacecraft came over Australia, Gemini 12’s hatch opened for the final time, and Aldrin conducted a second stand-up EVA. Lasting 55 minutes, this brought Aldrin’s total spacewalking time up to a record five hours and 30 minutes! Most of this EVA occurred as Gemini 12 passed over the night side of the Earth, so that Aldrin could aim his camera at “hot young stars”, which have stimulated the curiosity of astronomers all over the world. He also took numerous ultraviolet photographs of stars and constellations.

Mission Accomplished

After a spaceflight lasting 94 hours, 34 minutes and 31 seconds, Geminin 12 made the second computer-controlled re-entry of the programme, splashing down safely in the western Atlantic just three miles from their target, near the recovery aircraft carrier USS Wasp.

Captain Lovell and Major Aldrin have now been recovered and are on their way back to the United States for post-flight debriefing. But we already know that the Gemini 12 mission has been a fitting grand finale to the Gemini project, clearly demonstrating that NASA has achieved all the goals it set for the programme: it has now mastered rendezvous and docking, direct ascent to orbit rendezvous, long-duration spaceflight equivalent to the time of an Apollo lunar mission, and – the trickiest of all, as they discovered – the art of spacewalking.

We should not forget that Gemini has been a team effort, directly involving more than 25,000 people from NASA, the US Department of Defence, other government agencies, universities and research centres, industry and tracking station partners overseas. Everyone involved should feel great pride in the way spaceflight has been advanced in an amazingly short time.

Very soon, the manned Apollo programme will commence, and we can all hope that it will lead to a successful landing on the Moon before the end of this decade. But we should not forget that its success will stand on the shoulders of the Gemini programme.

Postscript

But where are the Russians in the race to the Moon? No Soviet manned flight has been announced since Voskhod 2 in March last year. Has the USSR withdrawn from the race? That seems unlikely, but why do they appear not to have attempted rendezvous and docking missions? Perhaps they have decided to use a different method of reaching the Moon, such as direct ascent, using a massive multi-stage rocket, without the need for orbital rendezvous? After all, as far as we can tell, they still have larger and more powerful rockets than Western nations. Only time will tell, but I think there are still many surprises in store from the USSR before either the East or West wins the Space Race!

(Want more exciting space stories?  Join us for Star Trek tomorrow night at 8:30 PM (Pacific AND Eastern — two showings)!!)

Here's the invitation!



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Science / Space Race

[September 18, 1966] Soaring Higher (Gemini 11)

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by Kaye Dee

Back in July, Gemini 10 accomplished an incredibly ambitious mission, and I wondered then what the next Gemini flight could do to top it. Now we know. In its three-day mission, Gemini 11 carried out a packed program: it made a direct ascent to its Agena target vehicle, soared even higher than its predecessor, conducted two EVAs and 12 different experiments, created artificial gravity and even performed the first computer-controlled return to Earth. I’m exhausted just listing all these highlights!


Gemini-11 prime and backup crews (L to R): William A. Anders, backup crew pilot; Richard F. Gordon Jr., prime crew pilot; Charles Conrad Jr. (foot on desk), prime crew command pilot; and Neil A. Armstrong, backup crew command pilot

Anchors Aweigh!

You could almost say that Gemini 11 has been a US Navy mission, since both its crew are naval officers. The Command Pilot, Commander Charles “Pete” Conrad Jr., was selected in the second astronaut group in 1962. He was previously the Pilot for the then-record breaking Gemini 5 mission, spending almost 8 days in space. Making his first spaceflight, Gemini 11 Pilot L.t Commander Richard “Dick” Gordon Jr. was part of NASA’s third astronaut intake in October 1963. Both men were previously naval aviators and test pilots.

There’s also a nod to the crew’s US Navy background in their mission patch, which was designed in Navy colours of blue and gold. The major milestones of the mission are indicated by stars. The first orbit rendezvous with the Agena is indicated by the tiny star on the line representing the mission’s low Earth orbit, while the actual docking is marked by the large star on the left. The star at the top marks the plan to reach a record high apogee, and the star on the right signifies Astronaut Gordon's spacewalk. The three events symbolised by the three large stars are also depicted visually, with representations of the docked Gemini 11 and Agena, a gold line representing the high apogee orbit and a spacewalking astronaut. The Roman numeral XI soars above the Earth from the launch site in Florida.

Preparing for Apollo

An important goal of Gemini 11 was to prove the feasibility of the plan for direct ascent rendezvous on Apollo lunar missions, in which a returning Lunar Module will lift off from the Moon’s surface to rendezvous with the Command Module as it passes overhead. To practice this technique, Gemini 11 would attempt to rendezvous directly with its Agena target vehicle on its first orbit, rather than taking around four orbits, as has been the case on earlier Gemini flights. To achieve this manoeuvre, the Atlas-Agena target vehicle had to launch within the desired time, while the Gemini itself had only a two-second launch window!

Present and future in one picture. As Gemini 11 lifts off from the Cape Kennedy Air Force Station's Launch Complex 19, the first Apollo Saturn V rocket is on Launch Complex 39A at Kennedy Space Centre. This Saturn V is a non-flight Facility Verification Vehicle that is being used for pad fit checks

Although technical issues twice delayed the launch, Gemini 11 finally lifted off exactly on time 12 September (US time): its target vehicle had been launched an hour and 37 minutes earlier. Manoeuvres for Gemini to catch up with the Agena began quickly, and before its first orbit had been completed, Gemini 11 was flying in formation with its target and ready to dock. The actual docking was achieved nine minutes after rendezvous, just one hour and 34 minutes after liftoff. With an achievement like this, it’s amazing to think that the first rendezvous between two orbiting spacecraft occurred only nine months ago! Unlike Gemini 10, the Gemini 11 docking consumed less fuel than expected and both Commander Conrad and Lt. Commander Gordon conducted two docking exercises with the Agena, before a final manoeuvre established the docked spacecraft in a 178 x 188 mile orbit.


After a first orbit rendezvous, Gemini 11 is docked with its Agena. The target vehicle's antenna is seen extending upwards

“Ride ‘em Cowboy”

The first Extra-Vehicular Activity of the mission occurred 24 hours after launch, when Astronaut Gordon left the spacecraft to begin a spacewalk that was scheduled to last about 105 minutes, while he remained tethered to Gemini 11 by a life support umbilical line. After setting up a movie camera and retrieving a micrometeorite experiment, the next task involved fastening a 100-foot tether, stored in the Agena's docking collar, to a docking bar on the Gemini's nose. These would be used for experiments in passive stabilisation and the first creation of artificial gravity in space (see below!)


"Ride 'em cowboy," said Gemini 11 Command Pilot Conrad as Astronaut Dick Gordon rested on the Agena target vehicle. This view was taken over the Atlantic Ocean at approximately 160 miles above Earth

Like previous Gemini EVAs, working in space for an extended period proved more tiring than in the simulations and Gordon became exhausted, overstressing his spacesuit’s life support system. After attaching the tether, he stopped to rest, sitting astride the Agena, like a cowboy riding a bucking bronco. Heavy perspiration inside the suit obscured the astronaut’s vision, virtually blinding his right eye and the faceplate of his helmet became fogged due to heavy breathing. As a result, the EVA was terminated, with Gordon spending just 21 minutes outside the spacecraft. 

Reaching New Heights

On 14 September, more than 40 hours into the mission, the Agena target vehicle’s primary propulsion system was fired for 25 seconds to thrust the docked spacecraft to a maximum altitude of 853 miles, establishing a new manned spaceflight altitude record! The Gemini 11 crew were enthralled by the spectacular view from this unprecedented vantage point. They particularly commented on the blueness of the water and marked curvature of the Earth below them.


Conrad and Gordon reached the maximum altitude of their high orbit over the southern hemisphere. As they looked west over the western half of Australia, Conrad said "We're looking straight down over Australia now. We have the whole southern part of the world out one window. Utterly fantastic."

After two orbits at this record-breaking altitude, completed in 3 hours, 23 minutes, Conrad and Gordon once again used the Agena’s engines to drive the joined spacecraft back down to their original low Earth orbit.

Standing Up in Space

On flight day three, Astronaut Gordon performed the mission’s second EVA, a “stand-up" spacewalk like that conducted on Gemini 10. Positioned in the open hatch, standing on his seat, Gordon spent two hours and eight minutes photographing the Earth, clouds and stars, as part of the range of experiments to be performed during the flight. During this period, Conrad manoeuvred the spacecraft to point Gordon and his camera in whatever direction was required. Unlike his first EVA experience, Gordon found the “stand-up” spacewalk so peaceful that he actually fell asleep!


Astronaut Dick Gordon stands in the open spacecraft hatch during the Gemini 11 mission

Inflight Experiments

The photography that Gordon undertook during his “stand-up” EVA were part of a packed program of 12 scientific experiments planned for Gemini 11. These included photography of the Earth for research in geology, geophysics, geography, oceanography, and related fields, and photography of clouds to study the fine structure of the Earth's weather system. Other experiments focused on astronomy and upper-atmosphere studies, while three experiments had specific military applications. There was a biological experiment looking at whether weightlessness enhances the effects of radiation on human white blood cells and Neurospora crassa fungi. An interesting photographic experiment investigated the regions of the L4 and L5 libration points of the Earth–Moon system. These are zones trailing and ahead of the Moon's orbit that are gravitationally stable. It is theorized that there might be clouds of particulate matter, or even tiny mini-Moons, which it is theorised may be orbiting the Earth in these regions.

Making Artificial Gravity!

After the stand-up EVA, 50 hours into the mission, Gemini 11 commenced a fascinating experiment in creating artificial gravity. Undocking from the Agena target vehicle, the Gemini 11 spacecraft slowly manoeuvred to stretch out the tether that Gordon had connected between them during his first spacewalk, and then allow the two tethered spacecraft to slowly rotate around one another.

The movement of the tethered spacecraft was first erratic, but stabilised after about 20 minutes, so that the rotation rate could then be increased. The astronauts found it challenging to keep the rope tether between the spacecraft tight, but they were able to demonstrate the "passive attitude stabilisation" of two spacecraft connected by a tether.


While tethered to their Agena target vehicle, the Gemini 11 crew manoeuvred their craft to keep the tether taut between the two. By firing their side thrusters to slowly rotate the combined spacecraft, they were able to use centrifugal force to generate about 0.00015 g of artificial gravity

The circular motion at the end of the tether created a slight artificial “gravitational acceleration” within Gemini 11. This is the first time artificial gravity has been demonstrated in space, even though that gravitational force was only 1.5 one-thousandths that of Earth. After about three hours, the rope tether was released, and the spacecraft moved apart.

Final Rendezvous

Although a fuel cell failed after the artificial gravity experiment, the remaining fuel cells were able to satisfactorily cope, and just under five hours before planned re-entry, Gemini 11 made a final “flyby” rendezvous with the Agena. This last rendezvous had not been part of the original flight plan but was made possible because of the fuel efficiency of the earlier rendezvous and docking manoeuvres. The fact that this rendezvous was made without use of the rendezvous radar, which had malfunctioned, is a testament to the skill and training of the Gemini 11 crew.


Gemini 11's Agena target vehicle seen during the "flyby" rendezvous. The tether from the artificial gravity and passive stabilisation experiment can be seen still attached to the vehicle

Coming Home Under Computer Control

Gemini 11’s return to Earth was the first fully automatic splashdown in the history of the US space program. On 15 September, at the end of its 44th orbit, Gemini 11’s retro-rockets were fired and the automatic re-entry was accomplished by computer commands directly to the thrusters. On earlier Gemini missions, the Command Pilot took controls of the re-entry at about 75 miles up, using the spacecraft's offset centre of gravity to generate lift for changes in direction. For Gemini 11, these manoeuvres were accomplished by computer commands. This process proved successful, and the capsule splashed down only 1.5 miles from the planned position in the Atlantic Ocean. A helicopter from the USS Guam picked up Conrad and Dick Gordon, taking the astronauts to the recovery ship.


Command Pilot Conrad climbs from Gemini 11 minutes after its successful computer-controlled splashdown

Heading to a Grand Finale

With Gemini 11, NASA demonstrated that it has has well and truly mastered rendezvous and docking. But the difficulties encountered by Lt Commander Gordon on his first EVA, and the problems that occurred on the spacewalks in previous missions, show that Extra-Vehicular Activity remains a challenge to be conquered. EVA is vital to the success of the Apollo programme, so Gemini 12, the final mission in this programme, will have spacewalking as its primary objective: it will be a grand finale indeed if Gemini 12 can demonstrate that the problems of EVA, like those of rendezvous and docking, have been successfully solved.




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Science / Space Race

[July 24, 1966] Doubling Up (Gemini 10)

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by Kaye Dee

A few days ago, Gemini 10 returned from the most ambitious US spaceflight to date. It literally took the Gemini programme to new heights and has firmly cemented the United States’ lead over the Soviet Union in the race to the Moon. Featuring not one, but two orbital rendezvous and two EVAs, Gemini 10 was a complex mission designed to increase NASA’s experience with these two techniques vital to the success of the Apollo lunar programme.

Designed by astronaut John Young’s wife Barbara, the Gemini 10 patch is simple, but highly symbolic. It features the Roman numeral 10 and two stars representing the two rendezvous attempts; Castor and Pollux (the two brightest stars in the constellation Gemini); and the two crew members. A stylized rendezvous is also depicted.

Crew for a Complex Mission

The Command Pilot for Gemini 10 was US Navy Commander John Young (left in the picture below), making his second spaceflight after acting as the Pilot of Gemini 3. Sitting in the right-hand seat as Pilot was US Air Force Major Michael Collins. A member of NASA’s third astronaut group, he is the first astronaut born outside the United States: his father is an Army officer and was stationed in Rome at the time of Collins’ birth.

Critical Timing

Blasting off on July 18, Gemini 10 was the first dual launch of a target vehicle and a manned Gemini flight to occurr exactly as planned. Launch timing was crucial, as Gemini 10 had only a 35-second window if it was going to rendezvous with two Agena targets in different orbits. The launch of the first rendezvous target, Agena 10, could not be delayed by more than 28 minutes, or it would result in a two-day wait until the second Agena already in orbit (originally launched for Gemini 8) would again be in position for the dual rendezvous plan to succeed. Agena 10 lifted off just two seconds late. One hundred minutes later it was followed by Gemini 10, launching exactly on time.

An amazing timelapse photo of Gemini 10's launch, showing the supporting rocker arm tower falling away

First Rendezvous

Despite the perfect launch, the path to Gemini 10’s first rendezvous was not completely smooth. An error made by John Young during the second burn – needed to rendezvous with the Agena about 160 miles above the Earth – required two additional burns to correct. By the time Gemini 10, on its fourth orbit, rendezvoused and docked with Agena 10, 60% of its fuel had been consumed. This placed constraints on the remainder of the mission, leading to the cancellation of several scheduled scientific experiments and additional docking practice.

Fortunately, the docking itself was successful and Mission Control decided to keep Gemini 10 docked to the Agena as long as possible. The target vehicle carried 3,400 pounds of fuel, some of which could be used for attitude control of the docked vehicles.


Docked to the nose of Agena 10, Gemini 10 Pilot Michael Collins took this impressive photograph of the Agena's engine firing as it boosted them to a record altitude

Rocketing to New Heights

Most of that fuel was needed for the second phase of Gemini 10’s mission. About seven and a half hours after launch, an 80 second burn of the Agena engine hurtled Young and Collins to an altitude of 474 miles, the farthest anyone has so far been from the Earth. This new record completely eclipses the previous record of 310 miles set by Voskhod 2 last year.

As the Gemini was docked nose-to-nose with the Agena, Young and Collins were flying ‘backwards’ as the rocket thrust them towards the higher altitude in a wild ride. Despite their unique vantage point, much of the view from the crew’s windows was blocked by the bulk of the Agena in front of them, so Young and Collins took very few photos: instead, they concentrated on their spacecraft’s instruments, especially the radiation dosage. The crew was particularly concerned about the radiation levels at their record-breaking altitude, as the lower edge of the inner Van Allen radiation belt was only about 150 miles above them. Fortunately, their instruments showed that the radiation levels at that altitude posed no danger to human life.


One of the few photos taken by the Gemini 10 crew at their record altitude, showing the curvature of the Earth. The Straits of Gibraltar are visible, with Europe to the left and North Africa to the right

Speaking of radiation, while Gemini 10 was orbiting aloft, France tested another nuclear weapon at Mururoa Atoll in the South Pacific. Although the astronauts were high too high above the blast zone for radiation to be an issue, Young and Collins were warned not to look at its blinding flash as they passed overhead.

When is a Spacewalk not a Spacewalk? When It’s a “Standup EVA”!

The Gemini crew began their second day in space with the news that they had enough fuel to complete the next phase of their mission, the rendezvous with Gemini 8’s Agena target vehicle. Another wild ride, pushed by Agena 10, lowered the Gemini to a new orbit with an apogee of 237 miles. Now the crew began to prepare for the mission’s first EVA, which would not see an astronaut actually leave the spacecraft. 

As an orbital sunset approached, Collins opened his hatch, exposing both astronauts to the space environment to perform a “standup EVA”. Standing in his seat with the upper part of his body outside the spacecraft, for a view unconstrained by its small windows, Collins commenced a photographic study of stellar ultraviolet radiation. He took 22 images of the southern Milky Way, scanning from Beta Crucis to Gamma Velorum (though, unfortunately, few of the images have proved scientifically usable). As Gemini 10 passed from night back to day, Collins also photographed a colour patch on the exterior of the spacecraft, to see if film could accurately reproduce colors in space. This task was cut short, though, when both Collins and Young experienced an eye irritation that caused their eyes to tear, making it difficult to see. As I write this article, the cause of this irritation is still uncertain, although it is thought to be a leak of lithium hydroxide in the environmental system.

Second Rendezvous

Gemini 10’s third day in space was its most complex and hazardous, commencing with the rendezvous with Agena 8. For the final time, Agena 10 fired its engine, to bring the docked spacecraft within 70 miles of Agena 8. At this point Gemini 10 discarded the Agena, which remains in orbit for use as a target by a future Gemini mission. Gemini 10 continued under its own power, for the first time in almost 48 hours, to reach Agena 8.

The former Gemini 8 target, having been in space since March, was essentially dead, without any power. Commander Young completed the critical final stage of rendezvous without the help of bright running lights and target radar, while trying to conserve enough fuel to let Collins take a one-hour spacewalk. He successfully guided the Gemini to within 10 feet of Agena 8, maintaining station close to the target vehicle without docking. This unique rendezvous simulated the rescue of astronauts from a spacecraft that had lost all electrical power.

A “Working” Spacewalk

With enough maneouvring fuel still available, Collins’ second EVA was now Go! Dubbed a “working spacewalk”, this EVA involved activities around the exterior of Gemini 10 and a traverse across to Agena 8. Like Gene Cernan on Gemini 9, Major Collins experienced difficulties in conducting his EVA tasks, demonstrating the need for more hand- and footholds on the exterior of future space vehicles. Nevertheless, he retrieved a micrometeorite collector from the exterior of the Gemini, containing experiments from Britain, Israel and West Germany. Unfortunately, this collector was later lost in space, apparently floating out of the spacecraft before the final hatch closing. 

Another micrometeorite collector was located on Agena 8. After one failed attempt to retrieve it, Collins used an experimental nitrogen-propelled “jet gun”, the Hand-Held Maneuvering Unit, to propel himself back to the Agena. This time he successfully retrieved the micrometeorite experiment, which is of particular scientific interest because of its long duration in orbit. There are no photos of the spacewalk available, but these training images give some idea of the complexity of the operations. However, low propellant quantity curtailed the spacewalk after only 39 minutes, instead of the originally planned hour. The crew experienced some difficulty in closing the hatch, due to the snake-like 50-foot umbilical used for Collins’ spacewalk and it was later jettisoned, along with the chestpack used by Collins and some other equipment an hour later. 

Return to Earth

About 63 hours into the flight, Young and Collins awoke to homecoming day, completing some final experiments, mostly involving photography of the Earth. Then, 70 hours and 10 minutes after liftoff, re-entry commenced and Young steered Gemini 10 to a pinpoint landing in the Atlantic only three and a half miles from the aiming point. The crew of the prime recovery vessel, the USS Guadalcanal, watched the spacecraft hit the water, as did millions of television viewers via the Early Bird satellite (though not us here in Australia, as we do not yet have access to satellite communications: it’s coming soon, though!).


For the first time the children of the recovery ship crew were allowed to be aboard to watch the splashdown and recovery. Here they join the party celebrating Gemini 10's safe return from a record-setting mission

Gemini 10 was certainly a mission for the record books: I can’t wait to see what further developments Gemini 11 will bring in just a couple of months’ time.




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Science / Space Race

[July 16, 1966] Onward and Upward! (Apollo, Australia, and OV)

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Not a month goes by without some interesting tidbits on the space front.  Even between Gemini and Voskhod missions, there's always something going on, all over the world!


by Gideon Marcus

Heavy Lifting

We are used to space shots being manned spectaculars — brave men in space suits heading into the cosmos.  But the missions that precede the human-crewed flights are just as important.  On February 26 of this year, we saw the first full Apollo test flight.  It featured an old-style Command Module, the bit of Apollo that will house crew, but the Service Module was standard production line.  The rocket, too, is going to see service.  Unlike the Saturn 1, which flew ten test flights in a row with remarkable reliability, the Saturn 1B will be used for actual Apollo missions, at least ones that will take place in Earth orbit.

The February flight, dubbed AS-201, was not without problems.  Nevertheless, it comprised a successful launch and landing after a 37-minute suborbital flight.

AS-203, launched July 5, was strictly a booster test.  The goal was to see if the Centaur second stage of the Saturn 1B could restart successfully in orbit, a critical function for lunar missions.  As a booster test, the rocket stack looked a bit odd.  Instead of an Apollo capsule, there was simply a nosecone covering the second stage.  The deletion of even a boilerplate also meant that the rocket could carry more fuel for testing.  By the time the vehicle had reached orbit, there was still 20,000 pounds of hydrogen and 3,000 pounds of oxygen in its tanks.

For four orbits, NASA engineers subjected the vehicle to various stress tests.  Hydrogen and oxygen were vented in various quantities.  In its final orbit, hydrogen was vented but the oxygen vents kept closed to create a tremendous pressure differential.  This eventually caused the rocket to explode, but not before surviving twice the expected endurance of the vehicle.  Call that a success!

Next up will be AS-202, which was bumped to accommodate this flight.  It will be a suborbital test like AS-201, but the Apollo will have fully functional guidance and navigation systems to test.  A few more successful flights, and we'll be on our way to the Moon!

Fraternal Twins

The Air Force has gotten a lot out of its budget "Orbiting Vehicle" program.  The idea behind the program was to utilize space on rocket test launches for satellites using standardized, mass-produced bodies.  This meant a double-savings over custom-built missions on mission-specific flights. 

Of course, things don't always work out as planned.  There are at least three OV series now, and only the OV2s have used spare test flights (in their case, on Titan 3Cs).  The OV3 series uses purpose-launched Scout rockets.  The OV1s, instead of using space on test-launched Atlas rockets (save for the first one), have instead used spare Atlases that were decommissioned from military service last year.  Still, the rockets were just sitting there, so it's still cheaper than it could have been.

In any event, OV1-7 and OV1-8, launched on July 14, represent the second time a pair of OV1 satellites were orbited back-to-back.  This particular launch was a little unusual for two reasons.  Firstly, OV1-7 (a standard OV1 satellite) was supposed to be a particle physics and "earthglow" detector. But it never left its Atlas and fell back to Earth.

Secondly, OV1-8 wasn't an OV1 at all, really.  It was a big balloon.  And not just an ordinary balloon: it was actually an aluminum grid put into spherical shape by being embedded in inflatable plastic.  When OV1-8 got to orbit, it inflated.  The Sun's rays disintegrated the plastic leaving a hollow mesh sphere.  Called PaGeos (Passive Geosynchronous), OV1-8 orbits the Earth at the same rate as its rotation, keeping it pretty much in the same spot in the sky with reference to a ground-based observer. 

And what good is a hollow aluminum balloon?  Why, for bouncing messages off of!  Turns out PaGeos reflects signals five times as well as the old NASA Project Echo balloons.  Also, the hollow nature makes PaGeos much less susceptible to air drag, which shortens the lifetime of a satellite by eventually pulling it down to Earth.  PaGeos was shot into orbit backwards to maximize air drag, yet it is calculated to have a lifespan of four years. 

Though active satellites like Telstar and Syncom have largely replaced passive balloon satellites, the cheapness and durability of passive comsats like PaGeos suggests there may be a specialized use for them in years to come.  I guess we'll just have to wait and see!


by Kaye Dee

(Not) Going Up from Down Under

Hello everyone, Kaye here. Gideon has kindly allowed me an opportunity to provide a quick update on recent space events in Australia. While the British and Australian sounding rocket programmes keep expanding, the European Launcher Development Organisation’s Europa launcher program at Woomera has had its first major failure-and one that was not the fault of the rocket itself!

Following the three successful test flights of the Blue Streak first stage, ELDO F-4 was intended to be the first all-up test of the three-stage Europa vehicle. The first stage was active, with the French second stage and the West German third stage inert dummies. The rocket was also carrying a dummy test satellite that carried some instrumentation to measure the conditions that a real satellite would experience during launch.

Although the 24 May lift-off went perfectly, the impact predictor soon reported that the rocket was veering west of the planned trajectory. At 136 seconds the Range Safety Officer terminated the flight, with the debris raiding down into the lower part of the Simpson Desert. To the disappointment of all involved, the post-flight analysis revealed that the rocket had, in fact, been exactly on course, and inaccurate readings had been received at the Mirikata downrange radar station 120 miles away. Oops! ELDO is now preparing for a new all-up test later this year, possibly in November. 

Waking a Sleeping Beauty

Australia has also recently played a special role in the Surveyor mission currently on the Moon. After the solar-powered probe shut down during the two week lunar night, the task of bringing it back to operational life was entrusted to the NASA Tidbinbilla Deep Space Tracking Station, outside Canberra. The re-awakening process on 8 July was a complete success and the space tracker who sent the "wake up" command was jokingly given a special citation: the Prince Charming Award!

[…and that's the space news for this week.  Stay tuned for full Gemini 10 coverage next week!]




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Book, Science / Space Race, Science Fiction/Fantasy

[June 12, 1966] Which Way to Outer Space? (New Writings In SF 8)

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by Mx. Kris Vyas-Myall

Space has been big news in the British press recently. Not the current struggles of America’s Gemini-9 link-up, but rather the saga of the UK’s presence in the ELDO.

ELDO logo

The European Launch Development Organization was formed by a treaty signed in 1962 between Britain, France, Germany, Italy, Belgium and The Netherlands for the development of a three-stage rocket launch for satellite use (you can read an excellent report Kaye Dee did on the project two years ago). However, the new British Labour government has been unhappy with the increasing costs and with the fact that Britain was paying around 40% of the cost rather than investing in its own rocket program, like some of the other nations have been.

The issue apparently came to a head when estimates for the Europa 1 launcher had risen to £150m, with no expectation of much practical use before 1969. For the last week negotiations had been happening feverishly to try to come up with a solution, with concerns that Britain would have no involvement in space in the future and the whole Eldo project could end up being scrapped.

ELDO launch brochure
Brochure for the upcoming Europa 1 launches from Woomera

Thankfully, a solution has been found. Britain will still be involved but their share of the cost will be reduced to 27%, whilst other countries shares increasing to meet this shortfall, making the payments between the largest countries more equitable.

New Writings in SF 8

Space is also the main theme of this quarter’s New Writings anthology, with new angles used to look at the familiar subject.

New Writings in SF8 Cover

Before we start on the stories, can we address the fact that these Dobson hardbacks are incredibly ugly to look at? They are just the same image and format reproduced in different colors each time. The Corgi paperback editions all have much more attractive covers which are likely to intrigue the reader:

Covers for New Writings anthologies 1, 2 & 3 in paperback from Corgi
The first three New Writings anthologies in paperback from Corgi

Could the publishers please make more effort? Or at least give us some variety after two years of the same dust jacket?

Anyway, on to the stories, let us see what Carnell’s crew comes up with:

The Pen and the Dark by Colin Kapp

We have the return of Kapp’s Unorthodox engineers for a third installment (one in Carnell’s New Worlds and the other in New Writings 3). These stories seem to have fans enough to encourage more tales in this world, although I have personally not been enamored by what has been presented so far.

This time the team go to investigate a strange phenomenon on the planet Ithica. An alien vessel had appeared there, then vanished, leaving a mysterious pillar of darkness. The whole area appears to defy their understanding of physics and so the team must investigate further.

I have read some people find the stilted, unnatural dialogue in this series as a great way to give his world depth. To me it is just irritating, as it does not stray far enough from our own language to read as much other than wooden. This was also compounded for me by the fact that it is filled to the brim with scientific jargon I struggled to understand. I have a suspicion it may have been made up, as they say at the end:

And even if they’d tried to tell us, I doubt our capacity to have understood. Try explain the uses and construction of a Dewar flask to an ant – and see who gets tired first.

However, what I did appreciate was the atmosphere of adventure into the unknown he creates which dragged me along this obscure journey. Perhaps more one for the Niven fans out there?

Three stars

Spacemen Live Forever by Gerald W. Page

Page is a new writer to me but has apparently had a couple of pieces published in the American magazines. Here he produces a very grim take on the long intergalactic voyage.

Torman Graylight is first officer on a ship transporting a sleeping population to a new planet. He is the only person awake apart from second officer Kelly. But when Kelly dies in an accident, Graylight’s loneliness gets the better of him and he decides to wake one of the sleepers. But will this be enough for the two of them to survive the years of travel through the void of space?

Whilst these kinds of grim nihilistic tales are not generally to my taste, I do appreciate the skill with which he presents the atmosphere, giving us a real sense of hopelessness and isolation.

Four Stars

The Final Solution by R. W. Mackelworth

Mackelworth also serves up a grim vignette, this one on the inherent self-destructiveness of fascism. In this future, human racial supremacists (closely modelled on Nazis) encounter another species with similar ideology on The Rose World. They decide to do a series of tests to determine racial hierarchy.

Even though short it is a very poignant and necessary piece on the ease with which militarism and racism can take over a society. The only parts that stop me from giving it a full five stars are that some of the elements (e.g., calling the alien leader Slan) and the ending make the story a little too explicit, but it is still a very strong short.

A high four stars

Computer’s Mate by John Rackham

Captain Sven Soren is piloting the Stellar One through the gaps between atoms as a means of breaching light-speed, with the first attempt to Vega. To achieve this, they need a massive computer to control the ship’s complex mechanisms. Coming with it is Grant Wilson, whose job is to care for the machine and act as the link between crew and computer.

Their first “star-jaunt” is a success, with them finding an Earth style world and its inhabitants. However, the crew are distrustful of Wilson as he himself acts like a computer and are unwilling to heed his warnings of the dangers ahead.

I have decidedly mixed feelings about this piece. Whilst it is nice to see a story about a mentally disabled person (particularly where he gets to be the hero, rather than a victim) the abuse of the rest of the crew because of his differences still feels out of place. There are also large sections which are just philosophizing on the nature of life and humanity, which can be interesting at times but often seem to be used at the expense of the women crew members. And whilst it is nice to see multiple women involved in spaceship operations, they are not really shown to do much that is positive.

I think I will go straight down the middle and give it three stars.

Tryst by John Baxter

On the outer reaches of an Asimov-esque galactic empire, there is a barren, nearly forgotten colonized world called Dismas. their only real link with the central imperium is an annual ship sent to help support the colony and bring back any saleable merchandise.

However, on this shipment all the boxes of equipment sent instead contain boxes of rose petals and the new machines are made from paper and foil. Even the ship in orbit is mysteriously deserted. The young rebellious Nicholas is sent to take the ship back to Centre and find out what has happened.

This is a thoroughly sensory story, beautifully described with a real sense of wonder and melancholy. Unfortunately, the ending was a bit of a disappointment for me and the only thing keeping it from a full five stars.

Four stars

Synth by Keith Roberts

And of course, at last we come to the obligatory Keith Roberts tale! This time making up the final third of the anthology. However, this piece does not seem to have any relation to the space theme of the rest of the book, rather being one of artificial intelligence.

In the twenty-second century, Megan Wingrove is named as a co-respondent in a major divorce case, between famous painter Henry Davenport and his wife Ira Davenport, with it being claimed Megan had an affair with Henry whilst working as their maid and Ira’s companion. What makes this case unusual is that Megan is a synth, a kind of advanced robot with an organic skin and muscle structure.

As well as seeking damages for mental anguish, Ira wants to have Megan destroyed for being dangerous and behaving immorally. We observe the case unfolding as they debate as to whether or not it is possible for a human to have a sexual relationship with a synth and whether a synth can be deemed to be responsible.

I was initially cynical that Keith Roberts would be able to do this kind of tale justice but he manages to produce both a really tense courtroom drama as well as delving into questions of consent and love. This story manages to be applicable to real life (you could see the same questions emerging in a similar situation with a domestic servant) whilst also being distinctly science fictional. He gives more thought to what it would mean for human emotions and longings to hit up against our technological capabilities than I can think of in any similar story.

I am as surprised as anyone to find myself giving a Keith Roberts story a full five stars!

Back to Earth

Readjusting their focus back to traditional science fictional subjects and having a nice mix of new and old talents has really brought out the best in Carnell’s anthology series. Here they put new perspectives on these subjects and come out with a marvelous selection. Even the stories I didn’t like as much I think may have more to do with my personal foibles than the quality of the writing.

Hopefully, this can continue in issue #9 and not regress to the poor state of affairs we saw in the prior collection.

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