The Cosmic Mirror
By Daniel Fischer
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Current mission news: MGS (latest pictures!) + Cassini + Stardust

25 years of manned spaceflight in Europe
began in 1978 with the Interkosmos launches of the Chech, Polish and (East) German cosmonauts Remek, Hermaszewski and J�hn: ESA News, BMBF PR, Welt.
Update # 259 of Monday, August 25, 2003
SIRTF is up! / Deadly space disaster in Brazil / Mars closer than in almost 60,000 years / Options for Hubble / Giant gas cloud in record quasar / Pluto mission in danger again!

Last "Great Observatory" in orbit: NASA's Space Infrared Telescope Facility

The launch came years late, but now the fourth and final "Great Observatory" satellite is in orbit: Early on August 25 a Delta 2 has launched NASA's SIRTF from Florida's Cape Canaveral Air Force Station. Flying eastward over the Atlantic Ocean, the new observatory entered an Earth-trailing orbit the first of its kind at about 43 minutes after launch. Five minutes later, the spacecraft separated from the Delta's second and final stage. At about 6:39 UTC, some 64 minutes after take-off, the NASA Deep Space Network station in Canberra, Australia received the first data from the spacecraft. "All systems are operating smoothly, and we couldn't be more delighted," said David Gallagher, project manager for the mission at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

The last of NASA's suite of Great Observatories, the Space Infrared Telescope Facility will use infrared detectors to pierce the dusty darkness enshrouding many of the universe's most fascinating objects, including brown dwarfs, planet-forming debris discs around stars and distant galaxies billions of light years away. Past Great Observatories include the Hubble Space Telescope, Chandra X-ray Observatory and Compton Gamma Ray Observatory. The two-and-one-half to five-year mission is an important bridge to NASA's Origins Program, which seeks to answer the questions: "Where did we come from? Are we alone?" In-orbit checkout and calibration is scheduled to last 60 days, followed by a 30-day science verification period, after which the observatory is expected to begin its regular science mission.

The spacecraft is unique in that it is smaller and lighter than past missions involving cryogenically cooled telescopes. In past missions, a vacuum shell surrounded the telescope like a thermos bottle, actively chilling the observatory and science instruments. On the SIRTF, the vacuum shell surrounds only the instrument chamber and the liquid helium tank. Engineers refer to this configuration as a "warm launch architecture." It means that much less coolant is needed, allowing for the use of a relatively smaller launch vehicle. In addition, it will permit the spacecraft to collect science data for up to five years, twice the length of the longest previous infrared mission. A new name for the Space Infrared Telescope Facility is expected to be announced about four months after launch, when the first images and science results will be released. The new name was selected after a worldwide contest with more than 7,000 entries.

KSC Release [JPL] (earlier, still earlier), the Status, the homepage and a Fact Sheet.
Coverage of Aug. 25: SN, S&T, FT, SC, BBC, CNN, ST, NZ. Aug. 24: ST. Aug. 23: NSU, SC, FT. Aug. 22: CSM, AFP. Aug. 21: New Sci. Aug. 20: AFP. Aug. 19: ST. Earlier: a RAS and Univ. of Sussex Press Releases, a KSC Status on SCISAT and SIRTF and Ast. on SIRTF and SMART.

SMART-1 launch slips well into September

Because of problems with an Indian satellite sharing the same Ariane 5, the launch of ESA's first lunar mission has been delayed repeatedly, and no new date has been announced: ESA (earlier, still earlier) and ISRO Press Releases and coverage of Aug. 19: BBC, NZ, NSU, BdW. Aug. 18: ST, AFP, BBC. Aug. 14: ST. Aug. 13: NZ. Aug. 12: AFP. Earlier: MPAe PR, ORF and Welt.
Ozone-watching Canadian satellite launched - on Aug. 12 SCISAT got in orbit on time: Homepage, KSC, CSA and Orbital Releases and coverage by CBC, SN, SC. ST. Earlier: Orbital PR.

Rocket disaster in Brazil kills 21 technicians

Brazil's ill-fated space program has been hit by its most devastating disaster - and one of the worst ever in rocket history worldwide - on August 22: The VLS-1 had been undergoing preparations for a launch from the Alcantara launch facility no sooner than August 25 when it suddenly exploded without warning. The explosion destroyed the $6.5-million rocket and the two small satellites it planned to launch; they were carrying positioning equipment, a communications transmitter and energy source. Brazilian officials say that 21 people, including a mix of military and civilian technicians, were killed in the explosion, and 20 more have been hospitalized, some in serious condition.

There was no initial word regarding what caused the explosion, but later is became clear that one of four solid-propellant booster rockets had ignited prematurely, for whatever reason. The explosion which also led to the collapse of the launch pad is the latest setback in Brazil's efforts to develop its own launch vehicle; two previous VLS-1 launches had failed within minutes of liftoff in 1997 and 1999. First word of the accident had come at about the same time as the head of the Brazilian Space Agency was holding a news conference with his Ukrainian counterpart about a deal to launch Ukrainian Cyclone rockets from Alcantara. Previously there had also been talk about launching Russia's Proton rocket from this remote launch site close to the equator.

Coverage on Aug. 24: SN, ST. Aug. 23: AFP, BBC, Rtr, RP. Aug. 22: SN, AP, AFP, ST, RP, NZ.

Japan's 1st satellite has reentered

on August 1 after 33½ years in orbit: ISAS Note, AP. ALEXIS 10 years in space: AeroAstro PR.
Fist glide test of SpaceShipOne from 14 km altitude: Status Report, ST, New Sci., SC.
X-43A return to flight no later than mid-November - NASA is holding its collective breath about the future of "air-breathing" engine technologies: SC.

As Mars comes closer than in 59,619 years, MGS data seem to rule out oceans in the past

On August 27 at 9:51 UTC Mars will reach its closest point to Earth during the current opposition when their centers will be a mere 55,758,006 kilometers apart - the last time the Red Planet came even closer was in 57,617 BC, when it passed within 55.718 million km of Earth. So far no major dust activity has been recorded, providing Earth-bound and orbit-based observers alike a particularly good view of Mars' albedo features. The scientific discovery of the month comes from the Mars Global Surveyor, though: Its thermal emission spectrometer has found no detectable carbonate signature in surface materials at scales ranging from three to 10 km during its six-year Mars mapping mission. However, the sensitive instrument could detect the mineral's ubiquitous presence in martian dust in quantities between two and five percent.

So carbonate has been found, but only trace amounts in dust and not in large outcroppings as originally suspected: This shows that the TES can see carbonates - if they are there - and that carbonates can exist on the surface today. The trace amounts that we see probably did not come from marine deposits derived from ancient martian oceans, but from the atmosphere interacting directly with dust: Tiny amounts of water in Mars' atmosphere can interact with the ubiquitous dust. So there is no evidence for oceans interacting with the big, thick atmosphere that many people have thought once existed there. The absence of massive regional concentrations of carbonates, like limestone rather points to a cold, frozen, icy Mars that has always been that way, as opposed to a warm, humid, ocean-bearing Mars sometime in the past.

NASA selects Phoenix as the first Mars Scout mission

NASA has on Aug. 4 selected Phoenix, an innovative and relatively low-cost mission, to study the red planet, as the first Mars Scout mission, scheduled for launch in 2007. Phoenix, designed to land in the high northern latitudes of Mars, will follow up on Mars Odyssey's spectacular discovery of near-surface water ice in such regions. It will land in terrain suspected of harboring as much as 80 percent water ice by volume within one foot of the surface, and conduct the first subsurface analysis of ice-bearing materials on another planet. The Phoenix lander includes an instrument suite designed to completely characterize the accessible ice, soil, rock, and local atmosphere using state-of-the-art methods. Included in the instrument payload are microscopic imaging systems capable of examining materials at scales down to 10 nanometers while others will investigate whether organic molecules are contained in ice or soil samples.

Upon final descent, an innovative camera system will photograph the Phoenix landing site just before it touches down in late 2008. A powerful robotic arm will dig down into the soil and ice-rich ground as deep at 3.3 feet, while imaging with a camera mounted on the arm itself. The lander for Phoenix had originally been built and being tested to fly as part of the 2001 Mars Surveyor Program, but the program was canceled after the Mars Polar Lander was lost upon landing near Mars' south pole in December 1999. Since then, the 2001 lander has been stored in a clean room at Lockheed Martin in Denver, managed by NASA's new Mars Exploration Program as a flight asset. Renamed Phoenix, it will now carry improved versions of UA panoramic cameras and a thermal evolved gas analyzer (TEGA) from the ill-fated Mars Polar Lander, as well as experiments that had been built and delivered for the 2001 Mars Surveyor Program.

M�ssbauer spectrometer misbehaves on Sprit; all other instruments on both MER do fine

The first in-flight checkouts of the science instruments and engineering cameras on NASA's twin Spirit and Opportunity spacecraft on their way to Mars have provided an assessment of the instruments' condition by early August - all 10 cameras on each spacecraft (3 science cameras and 7 engineering cameras on each) performed well, but one of the three spectrometers on Spirit returned data that did not fit the expected pattern. The other two spectrometers on Spirit and all three on Opportunity worked properly. The M�ssbauer spectrometer on Spirit is the one whose test data did not fit the pattern expected from normal operation. Some of the theories we had developed for what might be causing the anomalous behavior of the M�ssbauer instrument on Spirit have been eliminated by looking at the data from the one on Opportunity: The remaining theories focus on an apparent problem in movement of a mechanism within the instrument that rapidly vibrates a gamma-ray source back and forth.

"The M�ssbauer spectrometer on Spirit is working, and even if we don't come up with a way to improve its performance, we'll be able to get scientific information out of the data it sends us from Mars," says PI Steve Squyres: "But it's a very flexible instrument, with lots of parameters we can change. We have high hopes that over the coming months we'll be able to understand exactly what's happened to it and make adjustments that will improve its performance. And if the M�ssbauer spectrometer on Opportunity behaves on Mars the way it did today, we'll get beautiful data from that instrument." "All the engineering cameras are healthy," adds JPL imaging scientist Justin Maki: "We took two pictures with each engineering camera - 14 pictures from each spacecraft. Even when the cameras are in the dark, the images give characteristic signatures that let us know whether the electronics are working correctly." The science cameras on each rover also all performed flawlessly, and a spectrometer on each rover for identifying minerals from a distance, mini-TES, also worked perfectly on each rover.

Record approach to Earth: an earlier Sky & Tel. article with the numbers, earlier papers by Meeus (PDF) and Beish with more details, the most up-to-date collection of the best amateur pictures by the OAA (more collections can be found here under "Links"), a preview of HST observations, various press stuff & info files by Science@NASA (earlier), Plan. Soc., S&T, RAS (earlier), ESA, Ast., JPL and AIP and coverage on Aug. 25: WP, SF Gate, Dsc, SC (other story), RP. Aug. 24: RP, BBC, SC. Aug. 23: BBC. Aug. 22: S&T, AFP, SC (other story). Aug. 21: FT, CSM. Aug. 20: AFP. Aug. 19: RP. Aug. 17: Guardian, SC. Aug. 12: Nat'l Geog. Aug. 8: S&T, SC. Aug. 5: S&T.

Another cool view of Mars behind the Moon by Dantowitz. Public invited to suggest targets for MGS' MOC: JPL Release, Ast., FT. Mars reverses track in sky: SC. Mars vs. Earth: SC.

Watery past unlikely: JPL Release, Physics Web, New Sci., Ast., BBC, SC, ST, NZ, RP, Welt.

Hot spots on Mars give hunt for life new target - giant hollow towers of ice formed by steaming volcanic vents on Ross Island, Antarctica are providing clues about where to hunt for life on Mars: Univ. of Melbourne PR [SN, SR], New Sci., ABC, BdW. Mars moons result of disaster? SC.

First Scout selection: JPL, NASA, UA [SN, SR] and MPAe Press Releases, Ast., New Sci., Plan. Soc., SC, BBC, FT, Rocky Mtn. News, Virginian Pilot, ST.
Mars vs. Earth: SC. Cleaning up on Mars: SpaceRev. Mars Society convention: SC.

MER instrument tests: JPL Release, Cornell Status, ST, BBC, FT, AP, Wired. MER rehearsals: SC. Beagle weather expectations: ESA News.

New maps of Mars' soil water from Odyssey: LANL Release [SD], Ast., Dsc.

India's lunar plans go ahead

The prime minister of India has announced plans to develop that country's first unmanned mission to the Moon some time before 2008 but offered no specific timetable: ISRO Press Release, SC, ST. China's lunar ambitions: AFP.

Deep Space 1's spare ion engine kept running

in an unprecedented experiment on the ground, for 30,000+ hours in total: JPL Release. Hayabusa's engine at work: ISAS Release (earlier). ESA likes ion engines, too: ESA Release. And NASA will use them again: Boeing Release.

Ulysses sees galactic dust on the rise

Three times more stardust is now able to enter the Solar System as solar activity fades and the polarity of the Sun changes: ESA Science News (earlier, still earlier), Ast., New Sci., SC, NZ, Welt.

Three options for the fate of the Hubble Space Telescope

are being pondered by NASA after a high-ranking panel has delivered its report (much earlier than expected) following a public hearing on July 31. NASA's current plans are to extend the life of the HST to 2010 with one Space Shuttle servicing mission (SM 4) in 2005 or 2006. The plan is tentative pending the agency's return to flight process and the availability of Shuttle missions. NASA plans to eventually remove the HST from orbit and safely bring it down into the Pacific Ocean. The three options presented by the HST-JWST Transition Plan Review Panel, listed in order of priority, however are:
  • 1. Two additional Shuttle servicing missions, SM4 in about 2005 and SM5 in about 2010, in order to maximize the scientific productivity of the Hubble Space Telescope. The extended HST science program resulting from SM5 would only occur if the HST science was successful in a peer-reviewed competition with other new space astrophysics proposals.
  • 2. One Shuttle servicing mission, SM4, before the end of 2006, which would include replacement of HST gyros and installing improved instruments. In this scenario, the HST could be de-orbited, after science operations are no longer possible, by a propulsion device installed on the HST during SM4 or by an autonomous robotic system.
  • 3. If no Shuttle servicing missions are available, a robotic mission to install a propulsion module to bring the HST down in a controlled descent when science is no longer possible.
In addition, the panel described various ways to ensure maximum science return from the HST if none, one or two Shuttle servicing missions are available. "A lot of astronomers and NASA officials were astonished, when we said our report was ready just one week after our public meeting," says panel chair John Bahcall: "This was possible because we reached unanimous agreement on our conclusions very quickly; remarkable when you consider there were six independent-minded scientists on the panel. Our secret is we did our homework very thoroughly. Many people helped to educate us."
The Report, the Options, the panel's homepage, NASA and Berkeley Press Releases and coverage by Science, SN, SpaceRev, S&T, Ast., New Sci., BBC, FT, SC, ST.
Earlier: S&T, NSU, SpaceRev, Dsc., SC (earlier, other stories, mailbag), BBC, Welt; Grunsfeld's full statement [SN]. Still earlier: IHT.
Hubble's future a case for a Soyuz - or Orbital Recovery? SD, SR.

Progress for the SIM mission

Sub-atomic measurements were conducted for the first time within a Microarcsecond Metrology Testbed, a key technology test for the Space Interferometry mission: JPL Feature, Ast.
SIM's planet options - the mission sould be able to detect habitable planets near stars significantly more massive than the sun: OSU PR [SD].

Giant gas cloud of atoms formed in first stars in most distant quasar

Astronomers studying the most distant quasar yet found in the Universe have discovered a massive reservoir of gas containing atoms made in the cores of some of the first stars ever formed. The carbon-monoxide gas was revealed by the Very Large Array (VLA) and the Plateau de Bure radio interferometer. The gas, along with the young galaxy containing it, is seen as it was when the Universe was only one-sixteenth its current age, just emerging from the primeval "Dark Ages" before light could travel freely through the cosmos. The distant galaxy, dubbed J1148+5251, contains a bright quasar powered by a black hole at least a billion times more massive than the Sun. The galaxy - at z=6.42 - is seen as it was only 870 million years after the Big Bang. The Universe now is 13.7 billion years old. J1148+5251 would have been among the first luminous objects in the Universe.

The original atoms formed in the Universe within the first three minutes of the Big Bang were only hydrogen and helium. Carbon and oxygen - the atoms making up carbon monoxide - had to be made in the thermonuclear furnaces at the cores of the earliest stars. The carbon and oxygen atoms in the gas detected were made by some of the first stars ever formed, only about 650 million years after the Big Bang. In the next 200 million years or so, those stars - probably very different stars from those we see today - exploded as supernovae, spreading the carbon and oxygen out into space. Those atoms then cooled and combined into the carbon monoxide molecules detected with the radio telescopes. The discovery gives scientists a tantalizing direct view of one of the earliest galaxies in the young Universe, and raises questions about the nature of the first stars and how galaxies and quasars formed.

Combining the radio observations with data from optical telescopes shows that the transparent "bubble" around J1148+5251 is about 30 million light-years in diameter: This is direct evidence that we are seeing this object helping reionize the Universe. The amount of molecular gas in the galaxy - a mass more than 10 billion times that of the Sun - tells the scientists that things were happening quickly in the early Universe. This is as much mass as we see in big galaxies today, and it had little time, astronomically speaking, to accumulate. Also, the most popular theory for how big galaxies formed is that they were built up over long spans of time by multiple mergers of smaller galaxies: That's why it's so surprising to see such a massive galaxy so early in the Universe. Studies of J1148+5251 and other distant objects yet to be discovered will help scientists find the answers to their questions about the Universe's early stars and galaxies.

Papers by Walter & al. and Bertoldi & al., NRAO and MPIfR Press Releases and coverage by New Sci., Ast., CSM, NZ.

Iron found in the same quasar

confirming star formation since z > 10: a paper by Barth & al.

The Dark Age of the Universe

The Dark Age is the period between the time when the cosmic microwave background was emitted and the time when the evolution of structure in the universe led to the gravitational collapse of objects in which the first stars were formed: a review by Miralda-Escude. Galaxies with 4.8 < z < 5.8 imaged with the VLT - the Dark Age was just ending: ESO, PPARC Releases.
Lab searches for Dark Matter particles: a long review by Bernabei & al. Is the Universe a hologram? SciAm. New theory of time raises eyebrows: SC. Strange Universe: Slate.

7 x 1022 stars in the visible Universe

This is the latest extrapolation from statistics in the local Universe: ANU Press Release, AFP, SC, CNN, BBC, Guardian, RP.

ISS Update

The 250-page CAIB report will be released on Aug.26: an announcement and the Prelim. Recomm. #5 on on-board ascent imaging, an ESA Release on a good ISS viewing window for Europe, NASA Releases on the naming of an ISS Program Scientist and of Expedition 8 [SN] as well as on 1000 days of human presence on the station, a JPL Release on the naming of asteroids for the Columbia crew and coverage of Aug. 25: SN, USN&WR, AFP, SC, NZ. Aug. 24: WP. Aug. 23: ST, SC, CNN. Aug. 22: WP, AFP, FT, ST. Aug. 21: Nature, AFP, SC, ST. Aug. 20: SD, SC. Aug. 19: AFP, SC. Aug. 16: ST.
Aug. 15: FT. Aug. 14: ST. Aug. 13: S&T, Ast. FT. Aug. 11: ST, AFP, BBC, RP, NZ. Aug. 10: AP. Aug. 9: ST. Aug. 8: NZ. Aug. 7: SN, SC, ABC. Aug. 6: ST. Aug. 5: New Sci., SN, FT, AFP 2, 1, SC, ST 2, 1. Aug. 4: SF Gate, ST, RP. Aug. 1: AP, ST. July 31: WP, FT 2, 1, ST 2, 1. July 30: AP, ST. July 27: ST. July 26: WP, ST, AFP. July 24: ST.
Two options emerge for NASA's Orbital Space Plane, a winged vehicle versus a capsule - and the debate is far from over: SN, SpaceRev. OSP docking demonstrator DART passes design review: NASA Release.
1st Chinese manned flight reportedly set for October 10: SD, ST, FT. Earlier: SD (earlier), New Sci., BBC, AFP (earlier), Welt.

Atlas V chosen for New Horizons - and the Pluto mission is threatened again!

NASA has chosen the Atlas V expendable launch vehicle as the launch system for the proposed Pluto New Horizons mission scheduled for launch in January 2006 - but congress suddenly plans to cut $55 million from the New Frontiers program, which would seriously delay the launch and science return of New Horizons: a DPS mailing, coverage by SD, ST and SC of the planned cut and JHU [SD], NASA and LockMart Press Releases plus coverage by SN, ST and SC on the launcher choice.

Pentagon strips 7 launches from Boeing Delta 4 rocket as punishment for corporate mischief during the Evolved Expendable Launch Vehicle development: AFNS and Boeing Press Releases, FT, SN, WP, ST, SC.

Large CCD camera installed on Palomar Observatory telescope

The QUEST (Quasar Equatorial Survey Team) camera has an array of 112 CCDs and has been installed on Palomar Observatory's 48-inch Oschin Telescope in California: UI Press Release, Ast.

Largest robotic telescope (2 meters aperture) takes first pictures on La Palma: PPARC Release, homepage, BBC, S&T, Ast. Fate of Moscow's planetarium: S&T.

SALT now nearly complete - the Southern African Large Telescope will be the largest optical telescope in the Southern hemisphere: U. Wisconsin PR.

STRM30 data set greatly improves maps of Earth's land mass

located between 60 degrees north and 60 degrees south of the equator - the SRTM30 map matches the GTOPO30 resolution, but with its seamless quality, a leap in global-scale accuracy: JPL Release [SN].

The Big Blackout as seen from space and other implications: NOAA Release, APOD, SC.

MERIS pictures show Aral Sea shrinking - over the last 40 years it has evaporated back to half its original surface area: ESA Release, BBC.

Landsat problem remains unsolved - the failure of a crucial component on the craft's primary instrument has left data from all of June and most of July unavailable to scientists and other users: SN, SC.

Hot on the trail of Geminga

Astronomers using XMM-Newton have discovered a pair of X-ray tails, stretching 3 x 1012 km across the sky - they emanate from the mysterious neutron star known as Geminga: ESA Science News.

Close encounters between stars form X-ray emitting, double-star systems in dense globular star clusters, Chandra observations confirm: Chandra Release, Ast. Chandra to look for X-rays from Earth: Science@NASA.

Canada's fastest computer simulates galaxies, black holes - it will be used to test our understanding of astronomical phenomena ranging from the development of structure in the universe over 14 billion years to the development of new planets: U Toronto PR.

More images from GALEX

have been received, revealing hundreds of galaxies to expectant astronomers, providing the first batch of data on star formation that they had hoped for: JPL Release [SN, SR], Ast.

UHECRs from Gamma Ray Bursts? Gamma-ray bursts may generate the most energetic particles in the universe, known as the ultrahigh-energy cosmic rays: GSFC Release. Many GRBs go undetected: MIT Press Release. Amateur detects GRB afterglow before the pros: GSFC, MIT Releases, AAVSO Page, Ast., S&T.

A Chandra view of Messier 17 reveals hot gas flowing away from massive young stars in the center of the Horseshoe Nebula: Photo Release.

Court sets value of moon rocks

A federal court has decided that a collection of lunar rocks stolen by four people last year is worth a mere $5 million - this is the first time a dollar value has been attached to samples returned by the Apollo missions, and it means that the moon rock thieves will not go to jail after all: FT (other story), CollectSpace, ST.

There is a hole in asteroid Juno - AO surface maps show that Juno, like other asteroids, is misshapen rather than round, and that it has "sharp" edges: CfA Release, Ast., BdW. Some Perseids 2003 results: AstroFoto.

24 new names for planetary moons have been announced: S&T. Kuiperoid named Huya: ABC. Naming solar system bodies: SC, JPL. An NIR image of Jupiter by Gemini: Photo Release.

  • A lunation in time-lapse from amateur pictures: APOD.
  • Predicting earthquakes with satellites? Three possible methods: Science@NASA.
  • ESO boss president-elect of IAU - the International Astronomical Union has appointed Catherine Cesarsky as President Elect for 2003 to 2006: ESO PR. New IAU president takes over: NSU. EC comissioner for Research at the ESO VLT: ESO PR.


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Compiled and written by Daniel Fischer
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