Tag Archives: OSO

[November 12, 1967] Still in the Race! (Apollo-4, Surveyor-6, OSO-4 and Cosmos-186-188)



by Kaye Dee

As I noted in my previous article, October was such a busy month for space activity that I had to hold over several items for this month. But November has already provided us with plenty of space news as well. Even though both American and Soviet manned spaceflight is currently on hold while the investigations into their respective accidents continue, preparations for putting astronauts and cosmonauts on the Moon are ongoing and the Moon race is still on!

“Oh, it’s terrific, the building’s shaking!”

Opening the door to human lunar exploration needs an immensely powerful booster, and the successful launch of Apollo-4 a few days ago on 9 November has demonstrated that NASA has a rocket that is up to the task. Although the Saturn 1B rocket intended to loft Apollo Earth-orbiting missions has already been tested, Apollo-4 (also designated SA-501) marked the first flight of a complete Saturn V lunar launcher.

The sheer power of the massive rocket took everyone by surprise. When Apollo-4 took off from Pad 39A at the John F. Kennedy Space Centre, the sound pressure waves it generated rattled the new Launch Control Centre, three miles from the launch pad, causing dust to fall from the ceiling onto the launch controllers’ consoles. At the nearby Press Centre, ceiling tiles fell from the roof. Reporting live from the site, Walter Cronkite described the experience: “… our building’s shaking here. Our building’s shaking! Oh, it’s terrific, the building’s shaking! This big blast window is shaking! We’re holding it with our hands! Look at that rocket go into the clouds at 3000 feet! … You can see it… you can see it… oh the roar is terrific!”

Firing Room 1 in the Launch Control Centre at Kennedy Space Centre, under construction in early 1966. The Apollo-4 launch was controlled from here

Could it be that the sound of a Saturn V launch is one of the loudest noises, natural or artificial, ever heard by human beings? (Apart, perhaps, from the explosion of an atomic bomb?) I hope I’ll get the opportunity to hear, and see, a Saturn V launch for myself at some point in the future.

The Power for the Glory

Developed by Dr. Wernher von Braun’s team at NASA’s George C. Marshall Space Flight Centre, everything about the Saturn V is impressive. The 363-foot vehicle weighs 3,000-tons and the thrust of its first-stage motors alone is 71 million pounds! No wonder it rattled buildings miles away at liftoff!

The F-1 rocket motor, five of which power the Saturn V’s S1-C first stage, is the most powerful single combustion chamber liquid-propellant rocket engine so far developed (at least as far as we know, since whatever vehicle the USSR is developing for its lunar program could have even more powerful motors).

The launcher consists of three stages. The Boeing-built S1-C first stage, when fully fuelled with RP-1 kerosene and liquid oxygen, has a total mass of 4,881,000 pounds. Its five F-1 engines are arranged so that the four outer engines are gimballed, enabling them to turn so they can steer the rocket, while the fifth is fixed in position in the centre. Constructed by North American Aviation and weighing 1,060,000 pounds, the S-II second stage has five Rocketdyne-built cryogenic J-2 engines, powered by liquid hydrogen and liquid oxygen. They are arranged in a similar manner to the first stage engines, and also used for steering. The Saturn V’s S-IVB third stage has been built by the Douglas Aircraft Company and has a single J-2 engine using the same cryogenic fuel as the second stage. Fully fuelled, it weighs approximately 262,000 pounds. Guidance and telemetry systems for the rocket are contained within an instrument unit located on top of the third stage.

Soaring into the Future

This first Saturn V test flight has been tremendously important to the ultimate success of the Apollo programme, marking several necessary first steps: the first launch from Complex 39 at Cape Kennedy, built especially for Apollo; the first flight of the complete Apollo/Saturn V space vehicle; and the first test of Apollo Command Module’s performance re-entering the Earth's atmosphere at a velocity approximating that expected when returning from a lunar mission. In addition, the flight enabled testing of many modifications made to the Command Module in the wake of the January fire. This included the functioning of the thermal seals used in the new quick-release spacecraft hatch design.

 
Up, Up and Away!

Apollo-4 lifted off on schedule at 7am US Eastern time. Just 12 minutes later it successfully placed a Command and Service Module (CSM), weighing a record 278,885 pounds, into orbit 115 miles above the Earth. This is equivalent to the parking orbit that will be used during lunar missions to check out the spacecraft before it embarks for the Moon.

After two orbits, the third stage engine was re-ignited (itself another space first) to simulate the trans-lunar injection burn that will be used to send Apollo missions on their way to the Moon. This sent the spacecraft into an elliptical orbit with an apogee of 10,700 miles. Shortly afterwards, the CSM separated from the S-IVB stage and, after passing apogee, the Service Module engine was fired for 281 seconds to increase the re-entry speed to 36,639 feet per second, bringing the CSM into conditions simulating a return from the Moon.


An image of the Earth taken from an automatic camera on the Apollo-4 Command Module

After a successful re-entry, the Command Module splashed down approximately 10 miles from its target landing site in the North Pacific Ocean and was recovered by the aircraft carrier USS Bennington. The mission lasted just eight hours 36 minutes and 54 seconds (four minutes six seconds ahead of schedule!), but it successfully demonstrated all the major components of an Apollo mission, apart from the Lunar Module (which is still in development) that will make the actual landing on the Moon’s surface. In a special message of congratulations to the NASA team, President Johnson said the flight “symbolises the power this nation is harnessing for the peaceful exploration of space”.

Goodbye Lunar Orbiters…

While Apollo’s chariot was readied for its first test flight, NASA has continued its unmanned exploration of the Moon, to ensure a safe landing for the astronauts. In August, Gideon gave us an excellent summary of NASA’s Lunar Orbiter programme, the first three missions of which were designed to study potential Apollo landing sites. Lunar Orbiter-3, launched back in February this year, met its fate last month when the spacecraft was intentionally crashed into the lunar surface on 9 October. Despite the failure of its imaging system in March, Lunar Orbiter-3 was tracked from Earth for several months for lunar geodesy research and communication experiments. On 30 August, commands were sent to the spacecraft to circularise its orbit to 99 miles in order to simulate an Apollo trajectory.

Lunar Orbiter-3 image of the Moon's far side, showing the crater Tsiolkovski

Each Lunar Orbiter mission has been de-orbited so that it will not become a navigation hazard to future manned Apollo spacecraft. Consequently, before its manoeuvring thrusters were depleted, Lunar Orbiter 3 was commanded on 9 October to impact on the Moon, hitting the lunar surface at 14 degrees 36 minutes North latitude and 91 degrees 42 minutes West longitude. Co-incidentally, Lunar Orbiter-4, which failed back in July and could not be controlled, decayed naturally from orbit and impacted on the Moon on 6 October. Lunar Orbiter-5, launched in August, remains in orbit.

…Hello Surveyor 6

A month after the demise of the Lunar Orbiters, NASA’s Surveyor-6 probe has made a much softer landing on the lunar surface, achieving a “spot on” touchdown in the rugged Sinus Medii (Central Bay – it’s in the centre of the Moon's visible hemisphere) on 10 November (Australian time; 9 November in the US). This region is a potential site for the first Apollo landing, but since it appeared to be cratered and rocky, mission planners needed to know if its geological structure (different to the ‘plains’ areas where earlier Surveyor missions have landed) could support the weight of a manned Lunar Module.

Only an hour after landing safely, Surveyor-6 was operational and sent back pictures of a lunar cliff about a mile from its landing point, which has been described as “the most rugged feature we have yet seen on the Moon”. The first panoramas from Surveyor indicate that the landing site is not as rough as anticipated, and seems suitable for an Apollo landing.

Deep Space Network stations in Australia are helping to support the Surveyor-6 mission, as well as Surveyor-5, that landed in the Mare Tranquilitatis (Sea of Tranquillity) in September and is still operational. Hopefully both spacecraft will survive the next lunar night, commencing two weeks from now. NASA plans to send one more Surveyor probe to the Moon, in January, so look out for a review of the completed Surveyor programme early next year.

Watching the Sun for Astronaut Safety

With the Sun moving towards its maximum activity late next year or early in 1969, and likely to still be very active when the Apollo landing missions are occurring (assuming that the programme resumes some time within the next 12 months), NASA has wasted no time in launching another spacecraft in its Orbiting Solar Observatory (OSO) series, to help characterise the effects of solar activity in deep space. A NASA spokesman was recently quoted as saying that “A study of solar activity and its effect on Earth, aside from basic scientific interest, is necessary for a greater understanding of the space environment prior to manned flights to the Moon”.

OSO-4 under construction

Launched on 18 October, OSO-4 (also known as OSO-D) is the latest satellite developed under the leadership of Dr. Nancy Grace Roman, NASA’s first female executive, who is Chief of Astronomy and Solar Physics. The satellite is equipped to measure the direction and intensity of Ultraviolet, X-ray and Gamma radiation, not just from the Sun, but across the entire celestial sphere.

The OSO-4 spacecraft, like its predecessors, consists of a solar-cell covered “sail” section and a “wheel” section that spins about an axis perpendicular to the pointing direction of the sail. The sail carries a 75 pound payload of two instruments that are kept pointing on the centre of the Sun. The wheel carries a 100 pound payload of seven instruments and rotates once every two seconds. This rotation enables the instruments to scan the solar disc and atmosphere as well as other parts of the galaxy. The satellite’s extended arms give it greater axial stability.

Hopefully, OSO-4 will have a long lifespan, producing data as solar activity increases across the Sun’s cycle, and enhancing safety for the Apollo and Soviet crews who will venture beyond the protection of the van Allen belts on their way to the Moon.

What are the Soviets Up To?

The USSR has been remarkably quiet about its manned lunar programme. One could almost think that they had given up racing Apollo to the Moon, if not for the rumours and hints that constantly swirl around. Rumours abounded at the time of the tragically lost Soyuz-1 mission that it was intended to be a space spectacular, debuting in the Soyuz a new, much larger spacecraft which would participate in multiple rendezvous and docking manoeuvres, and possibly even crew transfers, with one or more other manned spacecraft.

Such a space feat has yet to occur, but the mysterious recent space missions of Cosmos-186 and 188 suggest that the Soviets have something of the sort in mind for the future, and are still quietly working to develop the techniques that they will need for lunar landing missions and/or a space station programme.

It Takes Two to Rendezvous

On 27 October, Cosmos-186 was launched into a low Earth orbit, with a perigee of 129 miles and an apogee of 146 miles and an orbital period of 88.7 minutes. Cosmos-187 was launched the following day, and there has been speculation that it was intended to be part of a rendezvous and docking demonstration with Cosmos-186 but was placed into an incorrect orbit. However, as is so often the case with Cosmos satellites, the Soviet authorities only described their missions as continuing studies of outer space and testing new systems, so the actual purpose of this mission remains a mystery.


A rare Soviet illustration of what is believed to be the Cosmos-186-188 docking

However, Cosmos-186 was joined by a companion on 30 October, when Cosmos-188 was placed into a very similar orbit with a separation of just 15 miles. This clearly demonstrates the precision with which the USSR can insert satellites into orbit. The two spacecraft then proceeded to perform the first fully automated space docking (unlike the manual dockings performed by Gemini missions from Gemini-8 onwards), just an hour after Cosmos-188 was launched. Soviet sources, and some electronic eavesdropping by the now-famous science class at Kettering Grammar School in England, using surprisingly unsophisticated equipment, indicate that Cosmos-186 was the ‘active’ partner in the docking. It used its onboard radar system to locate, approach and dock with the ‘passive’ Cosmos-188.

While the two spacecraft were mechanically docked, it seems that an electrical connection could not be made between them, and no other manoeuvres appear to have been carried out while Cosmos-186 and 188 were joined together. Perhaps there were technical issues surrounding the docking, but an onboard camera on Cosmos-186 did provide live (if rather low quality) television images of the rendezvous docking and separation, and some footage was publicly broadcast.

After three and a half hours docked together, the two satellites separated on command from the ground and continued to operate separately in orbit. Cosmos-186 made a soft-landing return to Earth on 31 October, lending credence to the speculations that it was testing out improvements to the Soyuz parachute system, while Cosmos-188 reportedly soft-landed on 2 November.

Speculating on Soviet Space Plans

Was Cosmos-186 a Soyuz-type vehicle, possibly testing out modifications made to prevent a recurrence of the re-entry parachute tangling that apparently led to the loss of Soyuz-1 and the death of Cosmonaut Komarov? Building on speculations from the time of the Soyuz-1 launch, there have even been suggestions that Cosmos-186, while unmanned, was a spacecraft large enough to hold a crew of five cosmonauts. There is also speculation that Cosmos-188 may have been the prototype of a new propulsion system for orbital operations. Does this mean, then, that the USSR is planning some kind of manned spaceflight feat in orbit to celebrate the 50th anniversary of the Communist Revolution? Or that it will soon attempt a circumlunar flight, to reach the Moon ahead of the United States?

Whatever their future plans may be, the automated rendezvous and docking of two unmanned spacecraft in Earth orbit shows that the USSR’s space technology is still advancing rapidly. The joint Cosmos 186-188 mission proves that it is possible to launch small components and assemble them in space to make a larger structure, even without the assistance of astronauts. This means that massive rockets like the Saturn V might not be required to construct space stations in orbit, or even undertake lunar missions, if the project is designed around assembling the lunar spacecraft in Earth orbit. Has the Cosmos 186-188 mission therefore been a hint of what the USSR's Moon programme will look like, in contrast to Apollo? Only time will tell…




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


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





[February 18, 1965] OSO Exciting!  (February 1965 Space Roundup)


by Gideon Marcus

Remember the early days of the Space Race, when launches came about once a month, and there was plenty of time to ruminate over the significance of each one?

Those days are long past, my friends.  Like every other aspect of this crazy modern world we live in, the pace of space missions is only accelerating.  Just look at this grab bag of space headlines, any one of which might have been front page news just a few years ago:

Staring at the Sun

Three years ago, NASA launched the first of its "Observatory Class" satellites, the 200 kg Orbiting Solar Observatory (OSO).  Its mission was unprecedented: to get the first long-term observations of the Sun in all of the frequencies of the electro-magnetic spectrum, not just the narrow windows visible from the Earth's surface.

For two years, OSO gazed at the Sun with its thirteen instruments, dutifully reporting its findings to the ground.  The observatory revolutionized our understanding of our neighborhood star, particularly in finding the correlation between solar flares and the little microflares that precede them. 

OSO 1 went silent last May.  Like nature, NASA abhors a vacuum — at least one without satellites floating through it!  So on February 3, 1965, OSO 2 sailed into orbit to pick up where its predecessor had left off.

The new observatory only has eight instruments, but given that the weight of the craft is similar to that of OSO 1, I have to believe the new load-out is intentional.  Moreover, OSO 2 has some neat developments.  Its Ultraviolet spectrometer, Solar x-ray and UV telescope, and White-light coronagraph are all mounted on the "sail" of the spacecraft, and they can scan the disk of the sun from end to end, like a TV camera.  That should allow for more precision in the measurements.

Also, OSO 2 has a digital telemetry system rather than the analog FM system of OSO 1.  Digital systems are far less prone to error, and more information can be sent over any given length of time.  The new system can dump 3 million bits of data in just 5.5 minutes.

Finally, OSO 2 is smarter — it can accept some 70 commands from the ground instead of just 8.  Just what NASA scientists do with those commands, I don't know.  Maybe OSO brews great coffee.

The most important thing about OSO 2 is the timing of its launch.  Every 11 years, the Sun completes an output cycle, warbling from active to inactive status.  1965 is the Solar minimum, and this year marks a concerted international effort to watch the Sun from many different vantage points to take advantage of the opportunity.

You can bet OSO 2 will have some interesting data for us come 1966!

Requiem for a Vanguard

Hands over hearts, folks.  On February 12, NASA announced that Vanguard 1 had gone silent, and the agency was finally turning off its 108 Mhz ground transceivers, set up during the International Geophysical Year.  The grapefruit-sized satellite, launched March 17, 1958, was the fourth satellite to be orbited.  It had been designed as a minimum space probe and, had its rocket worked in December 1957, would have been America's first satellite rather than its second.  Nevertheless, rugged little Vanguard 1 beat all of its successors for lifespan.  Sputniks and Explorers came and went.  Vanguards 2 and 3 shut off long ago.  Yet the grapefruit that the Naval Research Laboratory made kept going beep-beep, helping scientists on the ground measure the shape of the Earth from the wiggle and decay of Vanguard's orbit.

The satellite's cry had slowly become weaker as its solar cell-charged batteries failed.  Finally, some time last year, Vanguard could be heard no more, though NASA kept listening for several more months.  It's not all sad news, however: Vanguard 1 will remain in orbit for hundreds of years more, and it can still be optically tracked.  That means it still has a long, useful life ahead of it, even now that it is mute.

Whole World in its Eyes

Here's a little TIROS tidbit.  Remember TIROS 9?  The first weather satellite launched into a polar orbit so it can see the whole Earth once a day as the planet rotates underneath?

We now have the very first picture of the world's weather.  It won't be the last:

The joys of being regular

There was a time when space was a hit-and-miss affair.  Seemed every time I opened the paper, there was news of yet another rocket blowing up.  These days, we can practically take success for granted.  Ranger 7 broke a six mission losing streak, the first two Gemini launches went swimmingly, TIROS has gone nine for nine.

Similarly, the Saturn 1 rocket, the biggest booster ever made, has had an impeccable launch record.  The lift-off on February 16 kept the streak going; the eight engine monstrosity delivered what I believe is the biggest satellite ever to be put into orbit.

Called Pegasus, it is an enormous cylinder with giant panels affixed to either side.  The panels occupy some 2300 square feet, and their job is to measure the density of micrometeoroids in orbit over the course of a many-year lifespan.

It sounds pretty mundane when you reduce the mission to its bare essentials.  Pegasus is like a big fly-catcher, spending its orbit running into space rocks.  But it's not the experiment that's so exciting, but the idea that we can now loft giant structures with a single launch.  Imagine that Pegasus was actually a space station module, and that it's wings were solar panels.  Now imagine assembling a few of them together using a maneuverable spacecraft, perhaps a Gemini derivative…

Yes, America is just on the edge of being in the space construction business.

Scenes to Come

Yesterday (February 17, 1965), the eighth Ranger blasted off from Cape Kennedy, destination: Moon.  If we've truly reached an era of reliability, we can expect the craft to hit its target on the morning of the 20th.  Stay tuned — you'll read about it here first!




[March 24, 1963] Bumper Crop (A bounty of exciting space results)


by Gideon Marcus

February and March have been virtually barren of space shots, and if Gordo Cooper's Mercury flight gets postponed into May, April will be more of the same.  It's a terrible week to be a reporter on the space beat, right?

Wrong!

I've said it before and I'll say it again.  Rocket launches may make for good television, what with the fire, the smoke, and the stately ascent of an overgrown pencil into orbit…but the real excitement lies in the scientific results.  And this month has seen a tremendous harvest, expanding our knowledge of the heavens to new (pardon the pun) heights.  Enjoy this suite of stories, and tell me if I'm not right…

How hot is it?

Mariner 2 went silent more than two months ago, but scientists are still poring over the literal reams of data returned since its rendezvous with Venus.  The first interplanetary mission was a tremendous success, revealing a great deal about the Planet of Love, whose secrets were heretofore protected by distance and a shroud of clouds. 

Here's the biggie: Preliminary reports suggested that the surface temperature of "Earth's Twin" is more than 400 degrees Fahrenheit.  It turns out that was a conservative estimate.  In fact, the rocky, dry landscape of Venus swelters at 800 degrees — possibly even hotter than the day side of sun-baked first planet, Mercury.  It's because the planet's dense carbon dioxide atmosphere acts like a heat blanket.  There's no respite on the night side of the hot world either; the thick air spreads the temperatures out evenly.

Thus, virtually every story written about Venus has been rendered obsolete.  Will Mariner 3 destroy our conception of Mars, too?

Just checking the lights

On February 25, the Department of Defense turned little Solrad 1 back on after 22 months of being off-line.  The probe had been launched in conjunction with a navigation satellite, Transit, back in June 1960.  For weeks, it had provided our first measurements of the sun's X-ray output (energy in that wavelength being blocked by the Earth's atmosphere and, thus, undetectable from the ground).  DoD has given no explanation for why the probe has been reactivated, or why it was turned off in the first place.  Maybe there's a classified payload involved?

Radio News from the Great White Spacecraft

Last September, the Canadians launched their first satellite — the "top-sounder," Alouette, whose mission was to measure the radio-reflective regions of our atmosphere from above.  The results are in, and to any HAM or communications buff, its huge news.

It turns out that the boundaries of the ionosphere are rougher at higher latitudes than at lower latitudes.  Moreover, Alouette has determined that the Van Allen Belts, great girdles of radiation around our planet, dip closer to the Earth at higher latitudes.  This heats up the ionosphere and causes the roughness-causing instability. — the more active the electrons, the poorer the radio reflection.  Now we finally know why radio communication is less reliable way up north.  The next step will be learning how to compensate for this phenomenon so that communication, both civil and military, can be made more reliable.

Sun Stroke Warning

After a year in orbit, NASA's Orbiting Solar Observatory is still going strong, with 11 of 13 experiments still functioning.  The satellite has probably returned more scientifically useful data than all of the ground-based solar observatories to date (certainly in the UV and X Ray spectra, which is blocked by the atmosphere).

Moreover, OSO 1 has returned a startling result.  It turns out that solar flares, giant bursts of energy that affect the Earth's magnetic field, causing radio storms and aurorae, are preceded by little microflares.  The sequence and pattern of these precursors may be predictable, in which case, OSO will give excellent advance warning of these distruptive events.

Tax money at work, indeed!

Galaxy, Galaxy, Burning Bright

In the late 1950s, astronomers began discovering some of the brightest objects in the universe.  It wasn't their visible twinkle that impressed so much as their tremendous radio outbursts.  What could these mysterious "quasi-stellar sources" be?

Now we have a pretty good guess, thanks to a recent scientific paper.  Cal Tech observers using the Mt. Wilson and Mt. Palomar observatories turned their gaze to object 3C 273, a thirtheenth magnitude object in the constellation of Virgo.  It turns out that 3C 273's spectrum exhibits a tremendous "red shift," that is to say, all of the light coming from it has wavelengths stretched beyond what one would expect.  This is similar to the decrease in pitch of a railroad whistle as the engine zooms away from a listener.

The only way an object could have such a redshift is if it were of galactic proportions and receding from us at nearly 50,000 km/sec.  This would place it almost 200,000,000 light years away, making it one of the most distant (and therefore, oldest) objects ever identified.

At some point, astronomer Hubble's contention that the universe is expanding is likely to be confirmed.  These quasi-stellar objects ("quasars"?) therefore represent signposts from a very young, very tiny universe.  What exciting times we live in!

Five years of Beep, Beep

St. Patricks Day, 1958 — Vanguard 1 was the fourth satellite in orbit, but it was the first civilian satellite, and it is the oldest one to remain up there.  In fact, it is the only one of the 24 probes launched in the 1950s that still works.

What has a grapefruit-sized metal ball equipped with a radio beacon done for us?  Well, plenty, actually.  Because it has been tracked in orbit so long, not only have we learned quite a bit about the shape of the Earth (the variations in Vanguard's orbit are due to varying gravities on the Earth, the measurement of which is called "geodetics"), but the satellite's slow decay also tells us a lot about the density of the atmosphere several hundred miles up.

So, while Sputnik and Explorer might have had the first laughs, Vanguard looks likely to have the last for a good long time.

Telstar's little brother does us proud

RCA's Relay 1, launched in December, is America's second commercial communications satellite.  It ran into trouble immediately upon launch, its batteries producing too little current to operate its transmitter.  Turns out it was a faulty regulator on one of the transponders; the bright engineers switched to the back-up (this is why you carry a spare!), and Relay was broadcasting programs across the Atlantic by January.  660 orbits into its mission and 500 beamed programs later, NASA announces that Relay has completed all tests. 

Nevertheless, why abandon a perfectly good orbital TV station?  Relay will continue to be used to transmit shows transcontinentally, especially now that Telstar has finally gone silent (February 21).  There is even talk that Relay could broadcast the Tokyo Olympics in 1964, if it lasts that long!

In a sea of Blue, a drop of Red

On March 12, 3-12 at the Spring Recognition Dinner of Miracle Mile Association, in Los Angeles, Cal Tech President, Lee DuBridge, noted that the United States has put 118 probes into space, while the Russians have only lofted 34 (that we know of).  He also pointed out that virtually no scientific papers have resulted from the Soviets' "science satellites." 

As if in reply, on March 21 the Soviets finally, after 89 days without a space shot, launched Kosmos 13.  (To be fair, it's been kind of quiet on the American side, too).  The probe was described as designed to "continue outer space research."  No description of payload nor weight specifications were given.  Its orbit is one that allows it to cover much of the world.  While it may be that some of the Kosmos series are truly scientific probes, you can bet that, like America's Discoverer program, the Kosmos label is a blind to cover the Russians' use of spy satellites.  Oh well.  Turnabout is fair play, right?

[Next up, don't miss Mark Yon's spotlight of this month's New Worlds!  And if I saw you at Wondercon, do drop me a line…]




[March 7, 1962] Sunny side up!  (Orbiting Solar Observatory (OSO) #1)


by Gideon Marcus

Look up at the night sky, and what do you see?  Darkness and countless points of light.  Maybe a planet or two, brightly untwinkling in the black.  It is interesting that the sky should be black – after all, there are lots of photons (light particles) buzzing around the sky even after the sun has gone down.  You've got radio waves and x-rays.  Gamma rays, microwaves, and the shimmering veil of infrared – heat.  And yet, we can't see any of it.  Just the pinpricks of stars on the night's sheet.

Part of that is a biological limitation.  Our eyes only see a tiny window of the electromagnetic spectrum: from purple to red, the colors of the rainbow.  Some species of life see a bit further, into the ultraviolet or the infrared.  Only one species has crafted the ability to see beyond this range: humanity.  With our scintillators and geiger tubes and giant dishes, we can see waves of all kinds. 

Well, not quite.  You see, even with these detectors, we are still half blind.  The blanket of air covering the Earth blocks many wavelengths of photons from outer space: X Rays, Cosmic Rays, many wavelengths of Ultraviolet.  To see the truly unseeable, you have to go into orbit.

That's when we really can look at those points of light.  These are the stars, those busy factories of nuclear fusion, busily turning hydrogen into helium.  There are 100 billion in our galaxy, alone!  And we happen to have a lovely example just 93 million miles away, orders of magnitude closer than Alpha Centauri, the second nearest system.  While we have been observing the sun with our eyes for thousands of years, and with instruments for several hundred, these observations have always been hampered by the screening interference of the atmosphere.

Enter OSO – the Orbital Solar Observatory.  This 200kg spacecraft is the heaviest American science satellite to date, dwarfing all of the Explorer series of probes.  It is the first satellite launched devoted to the long-term study of the sun, in wavelengths you can't see from the Earth's surface.

There are 13 experiments on board the (appropriately) solar-powered craft including three X-Ray detectors, four Gamma Ray monitors, an ultraviolet sensor, several particle counters, and a dust sampler.  Not only will OSO be up in orbit for months, but it will be joined by successors in the series such that, for the next 11 years (a complete solar cycle of sunspot maximums and minimums), we will have continuous measurements of our star.  It is an unprecedented experiment, one which will tell us much about the nearest star and, by extension, the rest of the Galaxy's stars.

Not only that, but we will learn a great deal about solar storms and the hazards of radiation to human spaceflight.  This will give us a better idea of when and for how long it is safe for astronauts to travel in space, on the way to the Moon, for instance (NASA Director, James Webb, says he expects a landing by 1968!)

When will this ambitious project start?  Why…today, March 7, 1962, in fact!  It was launched from Cape Canaveral this morning, and to all indications, it is working flawlessly.  It is the kind of mission that won't get a lot of press, particularly when compared to the glory that cloaked Glenn's manned Mercury mission last month.  Nevertheless, I think OSO deserves attention and praise.  It constitutes a genuine leap in technology and it extends the eye of our race far above the clouds in a way no previous satellite has done. 

If they gave out Hugos for unmanned probes, this one would get my vote!

On the other hand, OSO-1 has plenty of competition for that award, and it's sure to get much more.  Tiros 4, the fourth weather satellite, joined its still-functioning older brother (#3) last month on the 8th, and there have been a few mystery military launches since then.  The President has clamped down on Air Force flights as of the beginning of the year, so I don't know much about them save that two were Discoverer film-based spy sats and one was a Samos live-TV spysat.  Another launch happened just today, but it was classified, and I know nothing else about it.  (It's ironic that the reason for the information clamp-down is that the Soviets accused us of employing surveillance satellites, and we're trying to hide it; I'm afraid the cat's already out of that bag!)

So stay tuned…there's more yet to come!