The Cosmic Mirror

of News events across the Universe

Archival Issues # 51 to 60, of July 28 to Oct. 17, 1997

Compiled and written by Daniel Fischer, Skyweek - older "Mirrors" in the Archive

Winner of the Star Award Logo and Space Views Award Logo in 1997!

Daniel Fischer is also the 1997 winner of the
Bruno-H.-Buergel-Preis of the Astronomische Gesellschaft


Also check out Astronomy Now's Breaking News and Florida Today's Online Space Today!
Current mission news: Pathfinder (DLR) + MGS (science!) + Cassini + Galileo

Update #60 of October 17th, 1997, at 15:30 UTC,
marking the first birthday of The Cosmic Mirror which started
on Oct. 10th, 1996 and was celebrated by NASA with some fireworks:

Cassini on its way to Saturn!

On the 10th day of the launch window, finally everything worked like clockwork: the weather, technology and law all cooperated, and the $3.3b Cassini mission got on its way to Saturn on October 15th, 1997. The final administrative hurdle had been taken when NASA had received the approval of the White House: all about the mission can be found on the large official web sites from NASA and ESA.

An interesting footnote to the debate and protests about the safety of the radioisotope batteries: A local newspaper put a Cassini representative (Steve Edberg, well known to amateur astronomers from his time with the International Halley Watch) and a leading protester at a table and had them debate for four hours.

Now the focus is finally on the mission itself - which starts with 7 years of "cruise", leading to a dramatic arrival in the Saturn system. Funding shortages have led to the sad decision to forgo any scientific observations during the Venus and Earth flybys or to visit any asteroid enroute, like Galileo did. However, after the 4 year baseline mission in orbit around Saturn as well as the Huygens probe mission are finished, an extended mission is thought possible.

Briefly noted:

Pathfinder's main transmitter is working again after 9 worrisome days at JPL: Now finally engineering data can be downloaded and the status of the aging Sagan Memorial Station be investigated! Meanwhile Sojourner, not having heard from Earth for a while, should have started driving autonomously - which turns the incident into yet another engineering adventure.

The Mars Global Surveyor has temporarily halted its aerobraking after strange things happened to the misaligned solar array (which at first had been pushed almost into the correct position!). And the MGS is also delivering preliminary Martian science data, including a new image!

Mir finally jettisoned the old Progress ship, making room for the new cargo craft already launched. And Atlantis is back - after having probably located the main leaks of the Spektr module when bursts of air were pumped in and debris floated out.

NASA has selected two new Small Explorer missions: HESSI (launch in 2000) will study flares on the Sun, GALEX (2001) galaxies in the UV. In case one of these missions runs into severe development trouble, BOLT could study gamma ray bursts. And there might also be a TWINS mission with two satellites taking 3-D images of the Earth's magnetosphere.

The 50th anniversary of the 'breaking of the sound barrier' on Oct. 14, 1947, has been celebrated widely - the first supersonic flight set the stage for the U.S. space program. Only one day before the anniversary Thrust SSC broke the sound barrier on the ground as well - but this time spin-offs for the rest of us are less likely...

In a nutshell: The - probably - most luminous star known has been imaged by Hubble's NICMOS camera, causing some excitement (and note the 55537 degrees C - what a precision... :-). / A bright meteor over Texas was seen in broad daylight on Oct. 9th. / A new large robotic telecope will become available in 1999.

A current picture of Hale-Bopp still shows jet activity. / The planned test of the MIRACL laser gun has been cancelled - perhaps forever. / Temperature measurements from space are important for climate studies. / And the HET telescope has been inaugurated.


Original documents from the 1950's regarding Sputnik 1 and its impact - both from the Soviet Union and the U.S. - have been collected in a long Florida Today Special Report (scroll forward to Oct. 4th)! See also a French site (which is multilingual!) and CNN's report.

Update # 59 of October 2nd, 1997, updated at 18:30 UTC

First MGS Mars close-ups published!

This afternoon NASA published the first close-up views of Mars from the MOC 2 camera on the MGS that were taken after Mars Orbit Insertion on Sept. 12th but before the aerobraking passes through the atmosphere began in earnest. During the past three weeks, the Mars Global Surveyor Orbiter Camera (MOC) has acquired about a dozen moderately high resolution images of Mars to improve the understanding of the exposure and focus control of the camera, in anticipation of mapping operations that will begin in March of next year.

Most of the images are of relatively poor quality, as the MGS spacecraft is not yet in the orbit for which the MOC was designed - and still the views are quite dramatic! Two of the best images have now been released in several versions, along with "context" frames derived from Viking Orbiter images. And even this ist just a sneak preview: MGS has been using atmospheric drag to reduce the size of its orbit for the past three weeks, and will achieve a circular orbit only 400 km (248 mi) above the surface early next year. Mapping operations begin in March 1998. At that time, MOC narrow angle images will be 5-10 times higher resolution than these pictures!

Mir/Atlantis EVA successful; new Mir computer installed

Joint operations of the Atlantis & Mir crews during mission STS-86 have been very smooth so far, following a successful 7th docking of shuttle Atlantis with the battered station. During an EVA last night space exposure experiments were retrieved and a big cap left outside that may one day be used to seal the suspected main rupture of Spektr. Even more important: Atlantis brought a new central computer to Mir which could go online today (although "new" is relative; the system is from the Salyut era).

Meanwhile the launch of the first components of the ISS is only 9 months away, and all 15 nations involved in the giant project have just finalized the assembly sequence: the FGB and Node 1 will be launched in June and July, the Service Module in December, 1998. Most important for Europe: Columbus goes already in October, 2002. No longer around to celebrate it, however, will be the German space agency: DARA ceased to exist Oct. 1st and is being re-integrated into the German Aerospace Research Establishment (DLR).

Ariane 5: Second launch attempt slipped to late October

This time failure is not an option ... The 2nd test flight of the Ariane 5 has now slipped to "Oct. 15th at the earliest" because the "final qualification of the flight program software will require two additional weeks to complete." Today it was even announced that the earliest possible launch date would be Oct. 28th, if not Nov. 4th. (Yahoo Deutschland) There is also an unofficial site devoted to the program which is recovering from the June 1996 disaster. Initially planned to be onboard Ariane 502 was an AMSAT satellite which was dropped because of stability concerns. Meanwhile the rebuilding of the lost Cluster satellites has begun.

Briefly noted:

October 4th marks the 40th anniversary of Sputnik 1, a reason for celebrations around the World (e.g. in Baikonur, Bonn and Cambridge) and reviews of the spacecraft and what it meant.

Following a special attitude change the Canadian RADARSAT is now observing Antarctica as no radar satellite could do before. The aim is to study changes to the ice cover of the continent.

The Lewis satellite was destroyed when it re-entered the atmosphere on Sept. 28th - contact to the experimental Earth observer had been lost soon after launch when a mis-firing thruster spun up the satellite.

In a nutshell: Future small missions to comets are reviewed here. / What Earth would look like as a Black Hole and related relativistic ideas have been studied in Austria where the results were presented at the annual Meeting of the AG in Innsbruck. / New images from ISO have been published as has been a new HST image of Betelgeuze (with a remarkable hot spot at one rotation pole). / And you can follow the development of the current El Nino from space.


Update # 58 of September 27th, 1997, at 19:45 UTC

Cosmological distance of GRB's proven?

New observations by Hubble and with groundbased radio telescope bolster the case for the 'cosmological hypothesis' of Gamma Ray Bursts, i.e. that they are millions, if not billions, of light years away. There is the discovery by Hubble that the optical afterglow of the Feb. 28 GRB is still there (as predicted by the relativistic fireball scenario and in contrast to the quick and total fading predicted by 'local' models) - and observations with the VLA and VLBA show that the fireball is expanding (other version of release), again in accordance with the fireball model. All this and much more was announced last week at a major GRB conference at the MSFC which reported daily on the news: Start here and follow all the links in the blue box!

MGS: Mars has a magnetic field

Only a few days in orbit, and already the Mars Global Surveyor has made a major discovery: clear evidence from MGS' magnetometer hints at a field of 1/800 the strength of Earth's. With Surveyor's aerobraking now under way, Hubble has looked again at Mars, finding signs of the changing seasons but nothing to worry about. Meanwhile Mars Pathfinder's Sojourner is exiting the 'Rock Garden' and has embarked on her longest trek yet. The results of the Pathfinder mission have been summarized (with countless links) in German.

Briefly noted:

The launch of Cassini has been set for Oct. 13, but the controversy about its RTGs is far from over. The aggressive opposition is being met by detailled rebuttals from Cassini's supporters, e.g. at the National Space Society (follow some of the links!), while other sites strive for detailled understanding (SEDS, Florida Today, etc.). Cassini itself can be watched on a webcam.

Yet another solar-terrestrial event is under way but NASA says, do not fear... Detailed documentation about the rivers of plasma inside the Sun can be found at Stanford, more on helioseismology learned from GONG and HiDHN.

Shuttle mission STS-86 is under way, close to docking with Mir - never before had the fate of a misson hung in the balance hours before liftoff, but Goldin declared Mir safe for a visit, following independent advice.

In a nutshell: Hale-Bopp is back in the news after a successful observation by Hubble, and there is more to report. An excellent collection of images has also turned up. / Pictures of the lunar eclipse of Sept. 16 have been published by ESO, Austrian students and ... well, see for yourself :-) / A high resolution map of the Earth has been created by the USGS. / The HST has found an isolated neutron star. / And great Earth images from SeaWIFS have been released.


Update # 57 of September 16th, 1997, at 16:20 UTC


Don't forget tonight's Total Lunar Eclipse (see also here and here), which is under way -
and will be broadcast on the Internet, e.g. from Australia (they've got clear skies right now)!

Mars Global Surveyor safely in orbit!

Wild cheers again at the JPL: The Mars Global Surveyor has entered its first orbit around Mars, already made some science observations, and will aerobrake into the final mapping orbit over the coming months, before starting the most complete mapping of Mars ever attempted. Even after one Martian year has passed, the MGS might still serve as a 'communications satellite' for landers.

Meanwhile the batteries of Sojourner are empty but this does not at all mean the end of the first Martian rover mission! The main disadvantage of having to rely completely on solar power is that further APXS measurements are now only possible in daytime when the higher temperatures mean more noise in the data. Sojourner is still strolling through the Rock Garden - while the Sagan Station's meteorological observations are critical for the Global Surveyor's aerobraking strategy.

The IAU Circulars are now on the web

And, for the first time, completely legally! Since the General Assembly of the International Astronomical Union in August, the current issues of the IAUC's are accessible to everyone on the net with only a few hours delay. This offer to the astronomical and amateur astronomical community is experimental and will be continued only if it doesn't lead to mass cancellations of IAUC subscriptions (which are an important source of income for this service!) and if there is no abuse of the copyrighted material.

The user surface is still somewhat confusing, but give it a try: Click here and enter the number 6743, then hit enter. This should give you a circular issued on Sept. 13th; on the top and bottom of the page you can click to further releases. There are even some historical issues available: Try "1" for the latest news - from 1922. Or enter "5000" for the famous IAUC on the launch of Hubble. The Cosmic Mirror congratulates the Central Bureau for Astronomical Telegrams and the IAU Comm. 6 (which oversees the CBAT) to its bold decision!

Briefly noted:

The next Atlantis launch to Mir, mission STS-86, is now planned for September 25th. Meanwhile the cosmonauts were unable to precisely locate the leak(s) of Spektr during their first EVA on Sept. 6th, had to endure several more failures of Mir's central computer - and were also scared by a piece of U.S. space junk coming closer than any other unrelated satellite in 11 years!

The launch of Cassini is being delayed to at least Oct. 13 because the Huygens probe has been damaged in late August. At this time Cassini and Huygens had just been mated to the Titan rocket, to which they have returned after the successful repair of the torn Huygens insulation. The heated debate about the safety of Cassini's RTGs is continuing, however, with sometimes bizarre claims being made. One radical Munich city council member, e.g., claims that after a launch failure of Cassini everyone on Earth would die...

News Capsules: The launch of the Lunar Prospector has been delayed to Nov. 23. / Hubble has discovered a huge crater on asteroid Vesta and amazing UV effects around a galactic central region. / The 99th launch of an Ariane was a success; on board were Eutelsat Hotbird 3 and Meteosat 3. / The Pentagon is pondering an anti-satellite laser test. / New ISO Images of the Hubble Deep Field have been released. / The FORTE s/c has been launched on Aug. 29th. / And new SOHO results shed light on the inner workings of the Sun.


Update #56 of August 27th, 1997, at 18:45 UTC

Lewis and ACE launched; Lewis in trouble

One more it holds true: triumph and tragedy are never far from each other in space technology... On August 22nd the 2nd launch attempt of the LMLV 1 rocket succeeded after a failure during the first launch and carried the Lewis satellite into orbit - where the spacecraft got into trouble just 4 days later, spinning wildly. It is unclear whether a recovery of the innovative Small Spacecraft (which is an Earth observer with a small astronomical payload as well) is possible.

More luck for the Advanced Composition Explorer (ACE) which was launched on August 25th. This spacecraft will be stationed in a Lagrangian point between Sun and Earth and study the composition of the solar wind with nine instruments. And yet another launch of a small satellite is imminent: FORTE, for Fast On-orbit Recording of Transient Events: It is an advanced radio frequency impulse detection and characterization experiment. Emphasis is on the measurement of electromagnetic pulses, primarily due to lightning. The Pegasus lauch is set for Aug. 28th.

Sagan Station, Sojourner still going strong after 50+ days

Having completed its primary mission of 30 days already in early August, both the Sagan Memorial Station and the Sojourner rover keep going and going - we are already deep into the extended mission. Last week the mission ran into some trouble when Sojourner got stuck in the rock garden and communications glitches prevented quick counter measures. No harm was done, though, and both spacecraft (or Marscraft, rather) continue to operate fine.

During the first 30 days about 1.2 Gbit of data were returned, including 9669 IMP and 384 rover camera images as well as 4 million weather measurements: The amount of data is twice than was was hoped for! New pictures were published today after a lengthy gap. The only instrument from which new information is slow in coming is the APXS - here lengthy recalibrations in the lab are necessary to get rid of the surprisingly strong influence of Mars' thin atmosphere on the soil and rock spectra. Eventually all information will be retrieved.

Meanwhile the Mars Global Surveyor is closing in on Mars - you can follow the progress in the current status reports. Most interesting news at the moment> the collection of images taken during approach has grown with three views from August 20th (also discussed here). So the MGS is already 4 times as successful as the Mars Observer which obtained precisely one Mars image... :-) For other funny aspects of Mars check out what Hollywood made of it.

And the Hubble constant is ... 73, really!

73 +/- 6 (statistical) +/- 8 (systematic) km/s/Mpc: This is the last result from the Hubble Space Telescope Key Project which tries to "determine the Hubble Constant, H0, to an accuracy of +/- 10%. This goal will be achieved by the systematic observations of Cepheid variable stars in approximately 20 galaxies using the Hubble Space Telescope." By now Cepheid distances to a dozen galaxies have been measured, both nearby ones and several in the Virgo and Fornax clusters.

All those galaxies are mere stepping stones, though: They are 'used' to calibrate an amazing number of secondary distance indicators which then extend the distance scale to distances large enough to measure the more or less pure Hubble expansion of the Universe. The 73 value - which first surfaced in the spring of 1996 - has grown more stable in the past year, and when the project finishes in 1998 all bets are that the 'real' value of Ho will be in that vicinity. What does all that mean?

Not much, unfortunately! If the density of the Universe were closed to the critical one, Ho=73 would mean that the age of the Cosmos is just 9 Gyr (10**9 years). That would be a clear contradiction to the established ages of the oldest stars and would call for a modification of the standard big bang model, probably by introducing the cosmological constant (want more math? :-). But if the density of the Universe is low, as many observations suggest, then the age of the Universe could be close to 12 Gyr, and may be marginally consistent with the oldest stars... (The Sidereal Times, newspaper of the 23rd General Assembly of the IAU, # 5, Aug. 22, 1997, p.1)

Briefly noted:

Trouble for Cassini - no more: A leak in its Titan 4B rocket threatened to delay the Saturn orbiter's launch on Oct. 6th. If the launch window (which ends on Nov. 4th) would have been missed, the arrival in the Saturn system could have been delayed by years beyond the planned 2004 timeframe. But a new test showed that the rocket is fine and the launch remains on target for the 6th. Meanwhile the NEAR flyby of Mathilde has been turned into a video - courtesy of J. Veverka, Cornell Univ.

Discovery observed Hale-Bopp: After its on-time launch and deployment of CRISTA, a German atmosphere research satellite, the crew found some time for astronomical observations: Here is more about this SWUIS experiment, and here are some Hale-Bopp images! The shuttle returned on Aug. 19th.

Meanwhile the new Mir crew succeeded with the the crucial spacewalks: On August 22nd the cosmonauts had no trouble reconnecting the Spektr solar arrays and inspecting the module's interior, though powering up Mir is a slow process. As expected the small breaches in Spektr's hull were not found from the inside - all hopes are now focused on a spacewalk on Sept. 3rd. In Russia preparations for an actual repair operation in October are underway, but even if reparing Spektr fully turns out to be impossible, the challenge alone would be a major learning experience for future ISS operations, the U.S. and Russian partners agree.

News Capsules: For the first time, Fluor has been found in interstellar space. A disk around a young star has been found in the radio by planetary discologist V. Mannings. A new instrument for Hubble has been selected, to go up in 2002.

Find out how strange is the universe and how old ist it? Watch Hubble split Mira or how the first 8.2-m telescope for the VLT takes shape. A new telescope for the South Pole has been delivered, while NASA scientists dream of building a warp drive.

The Heaven's Gate folks are back; fortunately there are still skeptics around. Another weird idea by R. Hoagland has been smashed! Have you ever wondered how to make money from asteroids? And you can help find the real aliens! And finally, look at a raw image of the Earth in the UV with an apparent 'mini-comet' disintegrating, to be found near the end of the new version of the Small Comets FAQ.


Update #55 of August 1st, 1997, at 18:00 UTC
Posted from the 29th DPS Meeting in Cambridge, Mass., U.S.A.

Comet Mysteries: one solved(?), two remain

A vast amount of data has been collected in the past two years on the bright comets Hyakutake and Hale-Bopp, with an unprecedented array of instruments. Never before in history, not even during the apparition of comet Halley a decade earlier, have astronomers had access to so many wavelengths at the same time. And Hale-Bopp could also be observed with this modern equipment over a wide range of distances from the Sun (from 7 to 1 AU), providing additional insights into the workings of comets when they approach.

The analysis of the flood of observations has just begun. Some results came fast, such as the discovery of molecules never seen in comets but now readily detected esp. in the sub-millimeter range (such as HCOOH, HNCO, HCCCN, H2CS, SO, SO2, HCO+, NH2CHO and CH3OCHO). Other molecules seem to have been detected, but are not yet identified. And understanding the temporal behavior of the production rates is another challenge: There could be indications of an inhomegeneous structure of the comet's nucleus, either a relic of its formation or the product of past perihelion passages of Hale-Bopp. Three of the major comet puzzles of 1996 and 1997, however, were

Briefly noted:

Access to thousands of astronomical abstracts and also many of the actual papers is provided by the NASA-funded (and free) Astrophysics Data System. Software support to track all kinds of planetary bodies can be obtained from the Moving Object Support System. And everything you ever wanted to know about stellar occultations has been collected by the Telescope Data Center.


Update #54 of July 31, 1997, at 22:25 UTC
Posted from the 29th DPS Meeting in Cambridge, Mass., U.S.A.

Pathfinder has discovered its own backshell!

At the weekly news conference Mike Malin announced today for the IMP team that a 2 m sized white object in about 1.2 km distance cannot be anything but the backshell of the lander that was jettisoned seconds before touchdown. The discovery was made when a series of 25 blue images had been taken of a certain area in order to achieve 'super-resolution', and in each one a bright spot appeared. There's nothing natural expected on Mars that is shining white.

Other news from the press conference:

Redshift 4.92: New cosmic distance record set!

An international team of astronomers has discovered the most distant galaxy found in the universe to date, by combining the unique sharpness of the images from NASA's Hubble Space Telescope with the light-collecting power of the W. M. Keck Telescopes -- with an Aadded boost from a gravitational lens in space. The measured redshift (z) of 4.92 puts the galaxy slightly farther away than a quasar known for some time at 4.90.

The results show the young galaxy is as far as 13 billion light-years from us, based on an estimated age for the universe of approximately 14 billion years - or insert its redshift of 4.92 into your favorite cosmological model (at such a high z value distances and ages depend critically on the adopted values for the Hubble and cosmological constant and so on).

In any case the high z places the galaxy far back in time during the "formative years" of galaxy birth and evolution, less than a billion years after the birth of the universe in the Big Bang in some world models.The detailed image shows that bright dense knots of massive stars power this object. Due to the firestorm of starbirth within it, the galaxy is intrinsically one of the brightest young galaxies in the universe, blazing with the brilliance of more than ten times our own Milky Way. (adopted from STScI PR #25 of July 30, 1997)

And again: "microfossils" in a meteorite claimed...

Almost to the day one year after the famous 'Mars meteorite news conference' another NASA scientist claims finding evidence of fossil life in a different meteorite. Mushroom-shaped structures and other possible fossilized biological structures have been found in a meteorite that fell on Australia one night in September 1969, said Richard B. Hoover at a conference.

The object in question is a rare type of space rock called a carbonaceous chondrite. Carbonaceous chondrites are unusually rich in water and carbon compounds, the atomic building blocks of living organisms: they also contain a surprising number of other organic molecules, and have peculiarly low density. No one was sure where the Australian carbonaceous chondrite came from - certainly not from Mars. It has a composition similar to that of a large asteroid, Ceres, and of Phobos, one of the two moons of Mars and possibly a captured asteroid.

The announcement at a major SPIE conference has been greeted with even more scepticism than the 'Mars meteorite' claims one year ago: There, at least, the NASA scientists had several lines of evidence and not just some electron microscope images. And one should not forget that microscopic evidence alone has led to various 'life signs in meteorites' claims over the past 30 years - none of which was ever confirmed... (San Francisco Examiner July 31, 1997)


Update #53 of July 31st, at 17:00 UTC
Posted from the 29th DPS Meeting in Cambridge, Mass., U.S.A.

Who's still believing in 51 Pegasi?

By the end of this year we should know for sure whether the first ever 'real' extrasolar planet reported, the one very close to the star 51 Pegasi, exists or not. David Gray, the stellar spectroscopist who sees indications for stellar oscillations and not radial velocity effects due to a planet in 51 Peg's spectrum (see Updates #38 and 45), defended his position well at the conference. And Bill Cochran (who himself has co-discovered another - undisputed - extrasolar planet and was to debate the 51 Peg issue with Gray) more or less agreed with Gray's position!

Grays conclusions center on the temporal behavior of the so-called spectral line bisector curvature of 51 Peg: The star's spectral line shape changes over time in a manner very characteristic of stellar oscillations. One can make up a model with gravity mode oscillations of 51 Peg's surface that reproduce the line shape changes almost perfectly. At least five groups of researchers are now waiting for the next good observing wind of the star (coming up this fall) and will throw the latest of spectroscopic technology at 51 Peg.

Gray, who as a purely 'stellar' astronomer has no stake in extrasolar planet research, made it clear that he only dismisses this one particular case. He has no problems with many other extrasolar planets reported for other stars, especially when the radial velocity amplitudes are really large. And Cochran reminded the audience of many other stars that show radial velocity effects looking like planet effects but which are known to be intrinsic pulsations. Even for the pulsating star, Delta Cephei, a companion was once claimed... (July 31, 1997)

Briefly noted:

There are now 53 Trans-Neptunian Objects known and 7 Centaurs (presumably escaped TNOs): The latest extrapolations place roughly 70 000 TNOs and 5000 Centaurs in our solar system, with diameters greater than 100 km. This is a lot: There are only about 230 asteroids of this size or larger in the main belt. The largest TNO discovered so far has a diamater of 760 km, by the way: The gap between the 'typical' TNOs of 100 to 500 km and Pluto is slowling closing. Meanwhile the supposed detection of ordinary comet nuclei in the Kuiper Belt is staying highly controversial. (Talk at the conference by R. Malhotra, July 30, 1997)

Further upgrades to the NEAT asteroid hunting system should make it possible to find more than 75% of all potentially Earth-threatening ateroids larger than 1 km within the next 10 years (and almost all of them by 2015). Just working temporarily with one camera the system has found an amazing number of asteroids, and two more cameras will probably be mounted to two other similar air force telescopes. So far the astronomers are only guests there (on 1-year contracts), but their cameras are so much better than the military ones that there are now plans to keep them installed permanently and to use them both for asteroid hunting and satellite tracking. (News conference at the conference by E. Helin, July 30, 1997)

The opacity of the Martian atmosphere is still not clear (no pun intended): The analysis of frequent HST observations of Mars' clouds and dustiness still yields values significantly below those reported by the Pathfinder IMP camera team. E.g. on July 9th the optical depth from dust in the Pathfinder area was found by Hubble to be about 0.2, with hardly any noticable clouds. The 20-30% discrepancy is unresolved. (News conference at the conference by P. James, July 30, 1997) Meanwhile Sojourner got stuck but is free again while it continues to circle the Sagan Memorial station. (Florida Today July 31, 1997)

Hale-Bopp's sodium tail remains a mystery: There are many attempts already to explain the phenomenon, ranging from the neutralization of ions in the plasma tail over a gas source at or near the nucleus to four different gas production processes possible in the dust tail. The neutral sodium (Na) abundance actually increases. down the tail - and the position of the Na tail relative to the ion and dust tail changed at least once from March to April. (News conference at the conference by J. Wilson, July 31, 1997)

Another astronaut will fly to Mir this September than was planned: David Wolf will have so serve as a back-up for spacewalks and has to fit into a specific kind of spacesuit - what Wendy Lawrence doesn't. (NASA News July 30, 1997) Meanwhile Mir commander Tsibliev has said in an interview that he is not only innocent of causing the dangerous Progress crash in June - but that his steering skills actually avoided a deadly crash of Progress into the Mir core module... (CNN Online July 30, 1997)


Update #52 of July 29th, 1997, at 20:00 UTC
Posted from the 29th DPS Meeting in Cambridge, Mass., U.S.A.

We almost understand Jupiter's Europa

The understanding of the inner workings of Jupiter's moon Europa has come a long way since it was first visited by the Galileo spacecraft a year ago. The question, however, is still not answered: All 'tantalizing evidence' notwithstanding there is no clear proof that Europa has a liquid ocean today nor even that there was one in the past. All surface features sighted by Galileo so far (some with 35 meters resolution) can be explained equally well by the action of just partially melted ice. And if the young age of the surface turns out to be incorrect (because we misunterstood the cratering processes in the outer solar solar system greatly) then it is even possible that Europa is a dead world since a billion years.

What we know about Europa from detailled Galileo observations and theoretical modelling is

Many of the details are still worked on, but there are already evolutionary scenarios on how ductile (or liquid) ice from below can break through the frozen crust, either in localized spots (which leads to the formation of pits or domes - this phenomenon is called diapirism) or along lines. In the latter case a ridge forms which can later turn into a triple band. Understanding the ridges is the most important work for the Europoligists because they dominate the moon's surface. (Talks by R. Pappalardo and others at the conference, July 29, 1997)

NASA's Goldin presents another package of bold visions

In spite of all the successes NASA has had this year and which may have made space exploration more popular among the public than anytime else in the past quarter century, NASA administrator Dan Goldin sees great trouble ahead - unless the agenc continues with the radical changes he initiated 5 years ago. Among the points he made last night during a dramatic address to hundreds of planetary scientists assembled here:
And Goldin reiterated his recent call for an interstellar mission, a futuristic spacecraft that should travel to a distance of 10 000 AU in relatively short time, return information not raw data (for which there would be no downlink capacity), would require no commanding from Earth whatsoever and use some wild propulsion system not even dreamt about... (Address during the 'Space Policy Night' at the conference, July 28, 1997)

Briefly noted:

Pathfinders batteries degrade: Almost a month after landing the Mars Pathfinder shows the first signs of ageing. Interestingly the Sojourner is still going strong. (CNN Online July 29, 1997)

SeaStar will fly on August 1st NASA announced today: this satellite from Orbital Sciences is carrying a NASA instrument which will deliver the first color images of the Earth on a global scale. (NASA News #161 of July 29, 1997)

Ice on the Moon remains unconfirmed: An attempt to reproduce the analysis of the Clementine radar experiments has not yielded any conclusive results so far - actually there is not even a confirmation of any radar power returned from the South polar region at all. The studies continue... (Progress report by R. Simpson at the conference, July 29, 1997)


Update #51 of July 28th, 1997, at 23:00 UTC
Posted from the 29th DPS Meeting in Cambridge, Mass., U.S.A.

Mathilde's low density remains a mystery

Why does the asteroid visited one month ago by the NEAR spacecraft have such a low density (see Update #49)? Further analysis has confirmed that the average density of this highly deformed body is only (1.3 +/- 0.2) g/cm**3: Mathilde's mass has already been determined to within 6% (it is 10**20 grams), and the volume of the body has been calculated as 73 000 km**3. Although only half of the asteroid was imaged by NEAR its shape could be modelled reasonably well, so that the uncertainty of the volume is only 20-30 % (and might be reduced further by radar observations; see below).

The expected density was about 2.5 g/cm**3, like the chondrite meteorites that the spectrum of Mathilde resembles closely (for experts: it's like a dehydrated C I or C M). The fact that the density is only half as big could in principle have three explanations:

The big mystery, however, is: How did Mathilde become what it is today? It has many more big impact craters than the other two main-belt asteroids studied so far (Gaspra and Ida), with several close to the limit where the impacting body would have destroyed Mathilde (one is 33 km wide and 6 km deep!) and an extremely slow rotation (17 days).

Shouldn't the impacts have destroyed Mathilde alltogether - or rather have fused the boulders together? And shouldn't there be a satellite that could have slowed the rotation period (which 'normally' would be 5 to 15 hours) to the present value? NEAR undertook a dedicated search for such satellites when it receded from Mathilde but came up empty. And so the most successful asteroid flyby of all three (the optical navigation went perfect, despite all odds; more than 300 of the 534 images taken actually show Mathilde) has once more demonstrated how little we actually know about minor planets. (Talk and news conference at the conference by J. Veverka, July 28th, 1997)

Near Earth Asteroids - reshaped by planetary tides?

How did the Near Earth Asteroid 1620 Geographos get its extremely elongated shape? With a ratio of 3:1 of the long to the short axis and a rotation period of 5.2 hrs the body is close to flying apart. And that's probably what actually happened during a very close passage of Geographos to the Earth in the past, say computer simulations presented in a dramatic video at the conference.

Building upon earlier work Bill Bottke has simulated Geographos as a body with a 'typical' shape (axis ratio 1.8:1, 2 g/cm**3, 6 hrs spin period), built from 247 particles held together only by gravity. This 'body' was then sent close to the Earth, where three things could happen:

Did the 'Vesta chips' weather? About 20 asteroids are known with orbital elements similar to the big asteroid Vesta that also have very similar spectra - in the visible light, that is. In the Near-IR, however, they are much redder than Vesta: This probably means that these 'Vesta chips' have suffered from 'space weathering.' Or aren't these bodies related to Vesta at all? Nowhere else, however, in the asteroid belt, are asteroids with optical spectra so similar to Vesta, which makes a common origin likely. (Talk at the conference by T. Burbine, July 28, 1997)

Arecibo radar measurements of Mathilde are planned this fall: As one of the first asteroids of this program after the upgrade of the Arecibo antenna Steve Ostro is planning to observe NEAR's first asteroid Mathilde this November. The radar images should allow to arrive at a much better value of the volume of the asteroid (with an error of only 9%) and thus a better density - if the (largely unknown) rotation state of Mathilde allows for a complete mapping (and the telescope is working all the time). If the observations run into trouble there are more opportunities in 2001 and 2014 - we just have to be patient... (Talk at the conference by S. Ostro, July 28, 1997)

Briefly noted:

No APXS spectrum of the rock Souffle was obtained by Mars Pathfinder's Sojourner which couldn't place the instrument properly - and the rover is already on the way to 'Mini Matterhorn'. (CNN Online July 28, 1987) Meanwhile the magnetic targets on Pathfinder are collecting large amounts of magnetic dust from the atmosphere, while the opacity of the atmosphere is staying at around 0.5, with variations between 0.57 and 0.4, often with a daily trend downward: that seems to be due to icy clouds forming overnight (visible in some as yet unpublished IMP images) that evaporate every morning. (Talk and news conference at the conference by P. Smith, July 28, 1997)

The age of the surface of the Jupiter moon Europa stays controversial: The only way to guess it is to count impact craters, and the time history (and even the present rate) of impacts is far from clear. Nonetheless good arguments can be made that at least some areas of Europa (notably the 'ice raft' region) are only 1 to 100 million years old. This is a small fraction of the total age of Europa (4.6 billion years) - which means to a geologist that Europa is active today and that the likelyhood of an ocean still being there below the icy crust is high. (News conference at the conference by C. Chapman, July 28, 1997)

A new powerful online ephemeris calculation system has been created at the Jet Propulsion Laboratory: The Solar System Dynamics package will generate custom ephemerides, visibility calculations, physical data and more.


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Compiled and written by Daniel Fischer (send me a mail to [email protected]!), Skyweek
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