Posted on by Fraser Cain

Experiments Chosen for Mars Science Laboratory

NASA has selected eight proposals to provide instrumentation and associated science investigations for the mobile Mars Science Laboratory (MSL) rover, scheduled for launch in 2009. Proposals selected today were submitted to NASA in response to an Announcement of Opportunity (AO) released in April.

The MSL mission, part of NASA’s Mars Exploration Program, will deliver a mobile laboratory to the surface of Mars to explore a local region as a potential habitat for past or present life. MSL will operate under its own power. It is expected to remain active for one Mars year, equal to two Earth years, after landing.

In addition to the instrumentation selected, MSL will carry a pulsed neutron source and detector for measuring hydrogen (including water), provided by the Russian Federal Space Agency. The project also will include a meteorological package and an ultraviolet sensor provided by the Spanish Ministry of Education and Science.

“This mission represents a tremendous leap forward in the exploration of Mars,” said NASA’s Deputy Associate Administrator for the Science Mission Directorate, Dr. Ghassem Asrar. “MSL is the next logical step beyond the twin Spirit and Opportunity rovers. It will use a unique set of analytical tools to study the red planet for over a year and unveil the past and present conditions for habitability of Mars,” Asrar said.

“The Mars Science Laboratory is an extremely capable system, and the selected instruments will bring an analytical laboratory to the martian surface for the first time since the Viking Landers over 25 years ago,” said Douglas McCuistion, Mars Exploration Program director at NASA Headquarters.

The selected proposals will conduct preliminary design studies to focus on how the instruments can be accommodated on the mobile platform, completed and delivered consistent with the mission schedule. NASA’s Jet Propulsion Laboratory (JPL), Pasadena, Calif., manages the MSL Project for the Science Mission Directorate.

Selected investigations and principal investigators:

— “Mars Science Laboratory Mast Camera,” Michael Malin, Malin Space Science Systems (MSSS), San Diego, Calif. Mast Camera will perform multi-spectral, stereo imaging at lengths ranging from kilometers to centimeters, and can acquire compressed high-definition video at 10 frames per second without the use of the rover computer.

— “ChemCam: Laser Induced Remote Sensing for Chemistry and Micro-Imaging,” Roger Wiens, Los Alamos National Laboratory, Los Alamos, N.M. ChemCam will ablate surface coatings from materials at standoff distances of up to 10 meters and measure elemental composition of underlying rocks and soils.

— “MAHLI: MArs HandLens Imager for the Mars Science Laboratory,” Kenneth Edgett, MSSS. MAHLI will image rocks, soil, frost and ice at resolutions 2.4 times better, and with a wider field of view, than the Microscopic Imager on the Mars Exploration Rovers.

— “The Alpha-Particle-X-ray-Spectrometer for Mars Science Laboratory (APXS),” Ralf Gellert, Max-Planck-Institute for Chemistry, Mainz, Germany. APXS will determine elemental abundance of rocks and soil. APXS will be provided by the Canadian Space Agency.

— “CheMin: An X-ray Diffraction/X-ray Fluorescence (XRD/XRF) instrument for definitive mineralogical analysis in the Analytical Laboratory of MSL,” David Blake, NASA’s Ames Research Center, Moffett Field, Calif. CheMin, will identify and quantify all minerals in complex natural samples such as basalts, evaporites and soils, one of the principle objectives of Mars Science Laboratory.

— “Radiation Assessment Detector (RAD),” Donald Hassler, Southwest Research Institute, Boulder, Colo. RAD will characterize the broad spectrum of radiation at the surface of Mars, an essential precursor to human exploration of the planet. RAD will be funded by the Exploration Systems Mission Directorate at NASA Headquarters.

— “Mars Descent Imager,” Michael Malin, MSSS. The Mars Descent Imager will produce high-resolution color-video imagery of the MSL descent and landing phase, providing geological context information, as well as allowing for precise landing-site determination.

— “Sample Analysis at Mars with an integrated suite consisting of a gas chromatograph mass spectrometer, and a tunable laser spectrometer (SAM),” Paul Mahaffy, NASA’s Goddard Space Flight Center, Greenbelt, Md. SAM will perform mineral and atmospheric analyses, detect a wide range of organic compounds and perform stable isotope analyses of organics and noble gases.

Original Source: NASA News Release

Posted on by Fraser Cain

Deep Impact Prepared for Launch

Launch and flight teams are in final preparations for the planned Jan. 12, 2005, liftoff from Cape Canaveral Air Force Station, Fla., of NASA’s Deep Impact spacecraft. The mission is designed for a six-month, one-way, 431 million kilometer (268 million mile) voyage. Deep Impact will deploy a probe that essentially will be “run over” by the nucleus of comet Tempel 1 at approximately 37,000 kilometers per hour (23,000 miles per hour).

“From central Florida to the surface of a comet in six months is almost instant gratification from a deep space mission viewpoint,” said Rick Grammier, Deep Impact project manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “It is going to be an exciting mission, and we can all witness its culmination together as Deep Impact provides the planet with its first man-made celestial fireworks on our nation’s birthday, July 4th.”

The fireworks will be courtesy of a 1-by-1 meter (39-by-39 inches) copper-fortified probe. It is designed to obliterate itself as it excavates a crater possibly large enough to swallow the Roman Coliseum. Before, during and after the demise of this 372-kilogram (820-pound) impactor, a nearby spacecraft will be watching the 6-kilometer-wide (3.7-mile) comet nucleus, collecting pictures and data of the event.

“We will be capturing the whole thing on the most powerful camera to fly in deep space,” said University of Maryland astronomy professor Dr. Michael A’Hearn, Deep Impact’s principal investigator. “We know so little about the structure of cometary nuclei that we need exceptional equipment to ensure that we capture the event, whatever the details of the impact turn out to be.”

Imagery and other data from the Deep Impact cameras will be sent back to Earth through the antennas of the Deep Space Network. But they will not be the only eyes on the prize. NASA’s Chandra, Hubble and Spitzer space telescopes will be observing from near-Earth space. Hundreds of miles below, professional and amateur astronomers on Earth will also be able to observe the material flying from the comet’s newly formed crater.

Deep Impact will provide a glimpse beneath the surface of a comet, where material and debris from the solar system’s formation remain relatively unchanged. Mission scientists are confident the project will answer basic questions about the formation of the solar system, by offering a better look at the nature and composition of the celestial travelers we call comets.

“Understanding conditions that lead to the formation of planets is a goal of NASA’s mission of exploration,” said Andy Dantzler, acting director of the Solar System division at NASA Headquarters, Washington, D.C. “Deep Impact is a bold, innovative and exciting mission which will attempt something never done before to try to uncover clues about our own origins.”

With a closing speed of about 37,000 kilometers per hour (23,000 miles per hour), what of the washing machine-sized impactor and its mountain-sized quarry?

“In the world of science, this is the astronomical equivalent of a 767 airliner running into a mosquito,” said Don Yeomans, a Deep Impact mission scientist at JPL. “It simply will not appreciably modify the comet’s orbital path. Comet Tempel 1 poses no threat to Earth now or in the foreseeable future.”

Ball Aerospace & Technologies in Boulder, Colo., built NASA’s Deep Impact spacecraft. It was shipped to Florida Oct. 17 to begin final preparations for launch.

Principal Investigator A’Hearn leads the mission from the University of Maryland, College Park. JPL manages the Deep Impact project for the Science Mission Directorate at NASA Headquarters. Deep Impact is a mission in NASA’s Discovery Program of moderately priced solar system exploration missions.

For more information about Deep Impact on the Internet, visit: http://www.nasa.gov/deepimpact.

For more information about NASA and agency programs on the Internet, visit: http://www.nasa.gov.

Original Source: NASA/JPL News Release

Posted on by Fraser Cain

Rovers Find Another Indication of Martian Water

Scientists have identified a water-signature mineral called goethite in bedrock that the NASA’s Mars rover Spirit examined in the “Columbia Hills,” one of the mission’s surest indicators yet for a wet history on Spirit’s side of Mars.

“Goethite, like the jarosite that Opportunity found on the other side of Mars, is strong evidence for water activity,” said Dr. Goestar Klingelhoefer of the University of Mainz, Germany, lead scientist for the iron-mineral analyzer on each rover, the Moessbauer spectrometer. Goethite forms only in the presence of water, whether in liquid, ice or gaseous form. Hematite, a mineral that had previously been identified in Columbia Hills bedrock, usually, but not always, forms in the presence of water.

The rovers’ main purpose is to look for geological evidence of whether their landing regions were ever wet and possibly hospitable to life. The successful results so far — with extended missions still underway — advance a NASA goal of continuing Mars exploration by robots and, eventually, by humans, said Doug McCuistion, Mars Exploration Program Director at NASA Headquarters.

Klingelhoefer presented the new results from a rock in the “West Spur” of Mars’ “Husband Hill” at a meeting of the American Geophysical Union in San Francisco this week.

Spirit has now driven past the West Spur to ascend Husband Hill itself. One remaining question is whether water was only underground or ever pooled above the surface, as it did at Opportunity’s site. “As we climb Husband Hill and characterize the rock record, we’ll be looking for additional evidence that the materials were modified by ground water and searching for textural, mineralogical and chemical evidence that the rocks were formed in or modified by surface water,” said Dr. Ray Arvidson of Washington University in St. Louis, deputy principal investigator for the rover instruments.

The amount of worrisome friction in Spirit’s right front wheel has been decreasing. Meanwhile, rover wranglers at NASA’s Jet Propulsion Laboratory in Pasadena, Calif., continue to minimize use of that wheel by often letting it drag while the other five wheels drive. “Babying that wheel seems to be helping,” said JPL’s Jim Erickson, rover project manager. Both rovers continue working in good health about eight months after their primary three-month missions. “Looks as though Spirit and Opportunity will still be with us when we celebrate the landing anniversaries in January,” Erickson said.

Opportunity has completed six months of inspecting the inside of “Endurance Crater” and is ready to resume exploration of the broad plains of the Meridiani region. It has recently seen frost and clouds marking the seasonal changes on Mars. At this week’s conference, rover science-team member Dr. Michael Wolff of the Brookfield, Wisconsin branch of the Boulder, Colorado-based Space Science Institute is reporting those and other atmospheric observations. “We’re seeing some spectacular clouds,” Wolff said. “They are a dramatic reminder that you have weather on Mars. Some days are cloudy. Some are clear.”

A portion of Mars’ water vapor is moving from the north pole toward the south pole during the current northern-summer and southern-winter period. The transient increase in atmospheric water at Meridiani, just south of the equator, plus low temperatures near the surface, contribute to appearance of the clouds and frost, Wolff said. Frost shows up some mornings on the rover itself. The possibility that it has a clumping effect on the accumulated dust on solar panels is under consideration as a factor in unexpected boosts of electric output from the panels.

As its last major endeavor inside Endurance Crater, Opportunity made a close inspection of rock layers exposed in a part of the crater wall called “Burns Cliff.” Dr. Steve Squyres of Cornell University, Ithaca, N.Y., principal investigator for the rover instruments, said, “In the lower portion of the cliff, the layers show very strong indications that they were last transported by wind, not by water like some layers higher up. The combination suggests that this was not a deep-water environment but more of a salt flat, alternately wet and dry.”

JPL has managed the Mars Exploration Rover project since it began in 2000. Images and additional information about the rovers and their discoveries are available on the Internet at http://www.nasa.gov/vision/universe/solarsystem/mer_main.html and at http://marsrovers.jpl.nasa.gov. Information about NASA and agency programs is available on the Web at http://www.nasa.gov.

Original Source: NASA/JPL News Release

Posted on by Fraser Cain

Cassini Flies Past Mysterious Titan Again

With a diameter of 5,150 kilometres, Titan is the largest of Saturn?s family of moons; it’s even bigger than the planets Mercury or Pluto. It has an atmosphere of orange-yellow smog composed mostly of nitrogen with an abundance of hydrocarbon organic compounds including methane; although, it seems to have very few clouds. On October 26, Cassini passed close to Titan revealing a first glimpse of the moon’s strange surface. It discovered a rugged yet level landscape with few craters, meaning that the planet must be geologically active. Mysterious oily flows of cryogenic ice ooze across the surface. Planetary scientists have been thrilled by the results so far.

Titan is cold. Its surface temperature is -180? C – way too cold for liquid water, yet it’s close to the triple point of methane, where this hydrocarbon gas can exist in all three physical states at its surface: solid ice, liquid or gaseous.

Cassini turned its Ultraviolet Imaging Spectrograph (UVIS) towards the star Spica (Alpha Virginis), then Lambda Scorpi, and for the next 8 hours observed the stars as they were obscured by Titan’s atmosphere. This sensitive instrument is different from other types of spectrometers because it can take both spectral and spatial readings. It’s particularly adept at determining the composition of gases. Spatial observations take a wide-by-narrow view, only one pixel tall and 60 pixels across. The spectral dimension is 1,024 pixels per spatial pixel. Additionally, it’s capable of taking so many images that it can create movies to show the ways in which this material is moved around by other forces. This provided a vertical profile of the main constituents of the atmospheric layers that have a similar temperature profile to the Earth.

Close approach occurred before Cassini passed up through Saturn’s ring plane, and returned some of the best close up images of the ring system to date. Then Cassini began using its radar to map part of Titan’s surface terrain at a small solar phase angle. The experiment was looking for signs of hot spots on the moon’s surface that would indicate the presence of active cryo-volcanoes, and even lighting in Titan’s atmosphere.

The 2.6-meter Huygens lander probe will separate from its mother ship on Christmas Eve, travelling towards Titan and entering the moon’s atmosphere on 14 January. Much of Huygens’s science will take place during its atmospheric decent, which will be relayed to Cassini, and then transmitted back to Earth’s waiting scientists and the media. If Huygens actually lands successfully on Titan, it’ll be a major bonus for the mission.

Huygens will be attempting to determine the origin of Titan’s molecular nitrogen atmosphere. Planetary scientists want to answer the question: “Is Titan’s atmosphere primordial (accumulated as Titan formed) or was it originally accreted as ammonia, which subsequently broke down to form nitrogen and hydrogen?”

If nitrogen from the solar nebula (out of which our Solar System formed) was the source of nitrogen on Titan, then the ratio of argon to nitrogen in the solar nebula should be preserved. Such a finding would mean that we have truly found a sample of the “original” planetary atmospheres of our Solar System

Huygens will also try to detect lightning on Titan. The extensive atmosphere of Titan may host Earth-like electrical storms and lightning. Although no evidence of lightning on Titan has been observed so far, the Cassini Huygens mission provides the opportunity to determine whether such lightning exists. In addition to the visual search for lightning, the study of plasma waves in the vicinity of Titan may offer another method. Lightning discharges a broad band of electromagnetic emission, part of which can propagate along magnetic field lines as whistler-mode emission.

By Science Correspondent Richard Pearson

Posted on by Fraser Cain

What’s Up This Week – Dec 13 – Dec 19, 2004

Image credit: George Varros
Monday, December 13 – Tonight will be one of the most hauntingly beautiful and most mysterious displays of celestial fireworks all year – the Geminid meteor shower. First noted in 1862 by Robert P. Greg in England, and B. V. Marsh and Prof. Alex C. Twining of the United States in independent studies, the annual appearance Geminid stream was weak, producing no more than a few per hour, but it has grown in intensity during the last century and a half. By 1877 astronomers were realizing a new annual shower was occurring with an hourly rate of about 14. At the turn of the century it had increased to an average of over 20, and by the 1930s from 40 to 70 per hour. Only eight years ago observers recorded an outstanding 110 per hour during a moonless night… And now it is moonless again!

So why are the Geminids such a mystery? Most meteor showers are historic, documented and recorded for hundred of years, and we know them as being cometary debris. When astronomers first began looking for the Geminids parent comet, they found none. After decades of searching, it wasn’t until October 11,1983 that Simon Green and John K. Davies, using data from NASA’s Infrared Astronomical Satellite, detected an orbital object that was the next night confirmed by Charles Kowal that matched the Geminid meteoroid stream. But this was no comet, it was an asteroid. Originally designated as 1983 TB, but later renamed 3200 Phaethon, this apparently rocky solar system member has a highly elliptical orbit that places it within 0.15 AU of the Sun about every year and half. But asteroids can’t fragment like a comet – or can they? Original hypothesis were that since Phaethon’s orbit passes through the asteroid belt, that it may have collided with other asteroids causing rocky debris. This sounded good, but the more we studied the more we realized the meteoroid “path” occurred when Phaethon neared the Sun. So now our asteroid is behaving like a comet, yet it doesn’t develop a tail.

So what exactly is this “thing”? Well, we do know that 3200 Phaethon orbits like a comet, yet has the spectral signature of an asteroid. By studying photographs of the meteor showers, scientists have determined that the meteors are more dense than cometary material and not as dense as asteroid fragments. This leads us to believe that Phaethon is probably an extinct comet that has gathered a thick layer of interplanetary dust during its travels, yet retains the ice-like nucleus. Until we are able to take physical samples of this “mystery”, we may never fully understand what Phaethon is, but we can fully appreciate the annual display it produces!

Thanks to the wide path of the stream, folks the world over get an opportunity to enjoy the show. The traditional peak time is tonight as soon as the constellation of Gemini appears around mid-evening and lasts through tomorrow morning. The radiant for the shower is right around bright star Castor, but meteors can originate from many points in the sky. From around 2:00 a.m. until dawn (when our local sky window is aimed directly into the stream) it is possible that we can see (animated clip by George Varros.) about one “shooting star” every 30 seconds. The most successful of observing nights are ones where you are comfortable, so be sure to use a reclining chair or pad the ground while looking up. Please get away from light sources when possible – it will triple the amount of meteors you see, dress warmly, take along refreshments and just enjoy the incredible and mysterious Geminids!

Tuesday, December 14 – So if you thought last night was great, then don’t plan on getting extra sleep tonight as we wait out the two-day old Moon to set and Orion to rise. Tonight we’re going to locate and explore Don Macholz tenth comet discovery – C/2004 Q2! This is definitely a “not to be missed” treat. Even the most modest of binoculars will reveal this spectacular comet. Located tonight on the Eridanus border you can easily locate Q2 by identifying the constellation of Lepus below Orion and simply sweeping the skies a short distance to the west. You cannot miss Macholz. It’s that bright and that easy!

Holding a rough magnitude of 5, Comet Macholz is visible to the naked eye at a dark site, but is sufficiently bright enough to be caught with small binoculars under less than perfect conditions. What can you expect to see? The coma (at the time of my observances prior to this article) is wonderfully huge and about the size of that great globular cluster, M13, yet it is definitely brighter! Veteran comet observers will appreciate its concentrated nucleus, extensive coma and twin dust and ion tails. For the novice, Macholz will indeed appear like a large, unresolvable globular cluster with a bright core, but look up, up and away at the stretch of tail. It’s the finest (in my humble opinion) since Ikeya/Zhang! If the constellation of Lepus is too low for your location, don’t worry. The wonderful Macholz will continue in the days ahead to climb northward until it reaches Taurus by month’s end. This one is awesome!

Wednesday, December 15, 2004 – For early evening viewers, tonight’s Moon will give a great opportunity to visit telescopically with some smaller features located within the fully disclosed Mare Crisium area. Near the terminator, look for two bright mountainous areas on the central western border of Crisium known as Olivium and Lavinium Promentoriums. Voyaging from this point toward the east across Crisium’s smooth floor, we will see the small punctuations of Craters Picard to the south and Pierce to the north. See how many nights you are still able to make out these features!

Thursday, December 16 – Tonight the Moon is once again our prominent sky feature, so why not venture there and visit one of the oldest features left on our visible lunar side? Start by identifying two prominent craters in the southeast quadrant – Metius and Fabricus. While viewing the area around these craters, note that Frabricus’ walls actually intrude upon Metius pointing to its younger age of formation. Around Fabricus, but not including Metius is the boundary of a mountain walled plain that extends into the terminator. High power and stable conditions will reveal many breaks in its hexagonal walls and its floor will be marred by many smaller craters and fissures. This is crater Jannsen, and in all probability is one of the oldest craters left on the Moon. Look for three prominent interior craters as well as an ancient rimae that will be at the shadow’s edge. It may not seem exciting, but remember crater Jannsen could be as much as five billion years old!

Friday, December 17 – As we continue our lunar exploration tonight, look for the “three ring circus” of easily identified craters Theophilus, Cyrillus and Catherina. It is here that you will find a very unique highlight – a very conspicuous lunar feature that was never officially named! Cutting its way across Mare Nectaris from Theophilus to shallow crater Beaumont in the south will appear a long, thin, bright line. What you are looking at is an example of lunar dorsum – nothing more than a wrinkle or low ridge. Chances are probably good that this ridge is just a “wave” in the lava flow that congealed when Mare Nectaris was formed and it is quite striking tonight because of the lighting angle. Has it been named? Yes. It is unofficially known as the “Dorsae Beaumont”, but whatever it may be called, it is surely a distinct feature that I think you’ll enjoy!

Saturday, December 18 – There’s still plenty of Moon to explore tonight, so why don’t we try locating an area where many lunar exploration missions made their mark? Binoculars will easily reveal the fully disclosed areas of Mare Serenitatis and Mare Tranquillitatis, and it is where these two vast lava plains converge that we will set our sites. Telescopically you will see a bright “peninsula” westward of where the two conjoin that extends toward the east, just off that look for bright and small crater Pliny. It is near this rather inconspicuous feature that the remains Ranger 6 lay forever preserved when it crashed on February 2, 1964. Unfortunately, technical errors occured and it was never able to transmit lunar pictures. Not so Ranger 8! On a very successful mission to the same relative area, this time we received 7137 “postcards from the Moon” in the last 23 minutes before hard landing. On the “softer side”, Surveyor 5 also touched down near this area safely after two days of malfunctions on September 10, 1967. Incredibly enough, the tiny Surveyor 5 endured temperatures of up to 283 degrees F, but was able to spectrographically analyze the area’s soil… And by the way, it also managed to televise an incredible 18,006 frames of “home movies” from its distant lunar locale.

Sunday, December 19 – Tonight’s outstanding lunar feature is easily seen in binoculars and a treasure-trove of detail to the telescope. Located roughly one-third the way from south to north limb, Crater Albategnius will stand out in bold relief near the terminator. A fine challenge for binoculars will be to see if you can make out its bright central peak from its darker lava covered floor. Telescopically, Albategnius is a real treat! Also an ancient formation, look for the large number of younger craters in its ruined walls. The largest of these is Crater Klein, but there are myriad others. A nice test of your optics and abilities to discern small features is to look for three shallow depressions east of the central peak. Good luck!

Until next week? Remember that many deep sky objects are still visible despite the Moon, so keep looking up and enjoying the wonders of our own Universe! Wishing you clear, dark skies and light speed… ~Tammy Plotner

Posted on by Fraser Cain

Work Begins on Magellan Giant Telescope

The Carnegie Observatories of the Carnegie Institution, and the University of Arizona, Steward Observatory Mirror Lab, have signed an agreement to produce the first mirror for the Giant Magellan Telescope (GMT)?the first telescope of the next-generation of extremely large ground-based telescopes ( ELT) to begin mirror production. The telescope primary mirror will have a diameter of 83 feet (25.4 meters) with more than 4.5 times the collecting area of any current optical telescope.

?This agreement is historic for the future of astronomy,? stated Dr. Richard Meserve, president of the Carnegie Institution. ?It is the first of many milestones that we and our partners look forward to?both in constructing an enormous ground-based telescope and in the scientific discoveries that will result. Everyone in the eight-member GMT consortium is extremely excited by this step,? he added. The consortium includes the Carnegie Observatories, Harvard University, Smithsonian Astrophysical Observatory, University of Arizona, University of Michigan, Massachusetts Institute of Technology, University of Texas at Austin, and Texas A&M University.

The GMT is slated for completion in 2016 at a site in Northern Chile. Viewing conditions in Chile, such as at Carnegie’s Las Campanas Observatory, are some of the best in the world. The GMT will have ten times the resolution of the Hubble Space Telescope. With its powerful resolution and enormous collecting area, the GMT will be able to probe the secrets of planets that have formed around other stars in the Milky Way, peer back in time toward the Big Bang with unprecedented clarity, delve into the nature of dark matter and dark energy, and explore the formation of black holes?the most important questions in astronomy today.

?The Giant Magellan Telescope will allow an unprecedented view of extrasolar planets as well as a window out to the largest scales and back to the earliest moments of the universe. We plan to complete the GMT so that it will work in tandem with the future generation of planned ground- and space-based telescopes,? stated Dr. Wendy Freedman, director of the Carnegie Observatories. ?The real distinction of the GMT, however, is that it is building on a heritage of successful technology developed for the twin 6.5-meter Magellan telescopes at Las Campanas. Their performance has far exceeded our expectations. The Magellan telescopes have proven to be the best natural imaging telescopes on the ground, due in large part to the genius of its Project Scientist, Carnegie Observatories? Stephen Shectman, and Roger Angel and his team at the Steward Mirror Lab,? she continued.

The mirrors for the GMT will be made using the existing infrastructure at Steward that made the 6.5-meter Magellan mirrors and the 8.4-meter Large Binocular Telescope mirrors on Mt. Graham. The new telescope will be composed of seven, 8.4-meter primary mirrors, arranged in a floral pattern. One spare off-axis mirror will also be made. Seven of the eight mirrors will be off-axis and require new techniques in casting and polishing. The first off-axis mirror will be cast this coming summer (2005) to address the new challenges. ?The upcoming decade promises to be a very exciting one for astronomy. The National Academy of Sciences Astronomy and Astrophysics Survey Committee Report (2001) ranked the science for extremely large telescopes as the highest priority for ground-based optical astronomy,? said Jeremy Mould, Director of the National Optical Astronomy Observatory. Site testing at the Las Campanas Observatory is also underway along with many other aspects of the project. Detailed information about the design of the GMT and the science that it will perform is located at http://www.gmto.org/.

Original Source: Carnegie News Release

Posted on by Fraser Cain

Dark Side of the Rings

As Cassini swung around to the dark side of the planet during its first close passage after orbit insertion, the intrepid spacecraft spied three ring moons whizzing around the planet.

Visible in this image are: Mimas (398 kilometers, or 247 miles across) brightest and above center; Janus (181 kilometers, or 112 miles across) second brightest at upper left; and Prometheus (102 kilometers, or 63 miles across) just above the main rings at upper left.

The normally bright B ring appears very dark from this vantage point. Regions with smaller concentrations of particles, such as the Cassini division (bright near center) transmit more sunlight and thus are brighter.

The image was taken in visible light with the Cassini spacecraft wide angle camera on Oct. 27, 2004, at a distance of 757,000 kilometers (470,000miles) from Saturn. The image scale is about 42 kilometers (26 miles) per pixel.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.

For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.

Original Source: NASA News Release

Posted on by Fraser Cain

NASA Administrator Set to Resign

NASA Administrator Sean O’Keefe is set to resign this week from the agency, after heading it up for three years. President Bush is considering five men to take over, with the former leader of the Pentagon Missile Defense Agency, Air Force Lt. Gen. Ronald Kadish, widely considered to be the top candidate. Other people being considered for the position are former Congressman Robert Walker and former shuttle astronauts Ron Sega, Charles Bolden and Robert Crippen. O’Keefe is said to be considering a new position as the chancellor of Louisiana State University.

Posted on by Mark Mortimer

Book Review: The Living Universe

Astrobiology is the study of life in the universe. It broadly encompasses many fields but purely for its own purposes. Early astrobiology (not that long ago) was, “a jumble of names with a variety of backgrounds and motivations and no central brain”. Its principal goal, to understand the inception of life, gave rise to many fundamental questions. What is life? How can or will we detect life on other worlds? How did life arise on Earth? What does life need to sustain itself? The questions were many and most still have no clear answer. As we read in this book, NASA had a strong influence in astrobiology in its early days and almost single handedly is keeping it going today.

Not all of the investigations related to astrobiology focussed directly on these lofty queries. For instance, space travel began and gave rise to the possibility of cross-planet contamination. Earth probes landing on foreign bodies (i.e. Viking) or especially when returning from foreign bodies (i.e. Apollo), shouldn’t transfer any harmful life forms. Other foretelling work included Stanley Miler’s experiment that simulated early Earth conditions and resulted in the formation of amino acids. Sidney Fox and his spherical proteinoids or Tom Cech and his RNA World thought they had tagged the beginnings of life in their own way though, not all agree. James Lovelock’s proposal, called Gaia, credited living things with having a dramatic effect on the atmospheric conditions on our planet. The early days were indeed a jumble, often supported by short term NASA contracts and almost always directed to space concepts. Nevertheless, a certain cohesion sprang up, together with the first moniker, exobiology.

Today’s investigations, well documented in the book, identify researchers and provide details relevant to the context of the day. The spectre of a hunt for little green men shadowed the creation of the SETI program and forced its evolution to an independent organization. The asteroid found in the Antarctic was blasted off from Mars billions of years ago and may have traces of life, but shapes tens of nanometres across leave a lot to the imagination. Nevertheless this finding may have assured the Viking and follow on programs that headed to Mars. The hunt for planets, difficult and error prone in the beginning, is now progressing rapidly, with indications that planets frequently occur. Again, throughout, NASA is shown to have a significant presence in these investigations, often supporting the inception stage and sponsoring many workshops and principal investigators. Also a name change happened as exobiology became astrobiology.

The destination of astrobiology is perhaps the most telling. A simple equation says it all. This equation known as the Drake equation, estimates the number of other technological civilizations in the galaxy. As long as this equation results with a value of one or greater, then there is at least one other life form to whom we can communicate. Obviously, if true, this could require a big change in some religions as well as some serious societal circumspections. But until we have the evidence, first contact will remain in the realm of science fiction. Reading between the lines, it appears that NASA is contemplating this question and considering options!

Our living universe is a fascinating subject with lofty goals. Dick and Strick do the history of the field justice by accumulating a description of so many of the activities, projects and workshops that relate to this topic. Sometimes the reading gets a bit dry. Typical passage are, ‘person x of department y at site z on date t did something’. Hundreds of names flow by, as well as contract descriptions, amounts, budgetary issues, personalities and the like. The style is more reminiscent of a memorial tomb than a Carl Sagan novel. Don’t be surprised by this as the funding for the book came from NASA. This does result in an apparent biassed result. For example, the first section of the book includes efforts from around the globe, while the remainder centres almost exclusively on NASA funded activities. Sometimes I got the feeling that this book was just a tool to justify NASA expenditures, which is a shame, as the subject is so interesting, and NASA has made a tremendous contribution. On the whole though, the book is well laid out, has only a few references to techno-speak and successfully covers a lot of information.

Hundreds of great scientists have contributed to astrobiology. This hunt for the understanding of life might be rationalized as the pursuit of knowledge for its own sake, or as a good preparation for contacting other worldly life. Either way, Steven Dick and James Strick in their book, The Living Universe – NASA and the development of Astrobiology, show the progress of these scientists and researchers and give credit to NASA’s support during the build up and implementation of this new research field.

Read more reviews, or order a copy online from Amazon.com.

Review by Mark Mortimer

Posted on by Fraser Cain

The Winter Solstice Approaches

Image credit: NASA
To understand the Winter Solstice (and by contrast the Summer Solstice) we must first understand a fundamental fact about the earth. Earth?s axis of rotation is tilted approximately 23.5? from vertical. This means that as earth orbits the sun, it points first one hemisphere, then the other toward the sun. This tilt causes sunlight to strike the surface of earth at different angles at different times of year. In the summer, the sun is high overhead for the Northern hemisphere and the heat energy is concentrated over a smaller area. In the winter, when the angle of the sun is low, the energy covers a much larger area and therefore heats less efficiently.

Imagine pointing a flashlight directly at a piece of paper. It’ll create a bright circle of light concentrated in an area. Now tilt the flashlight so that it’s hitting the paper on an angle. The same amount of light is coming out of the flashlight, but it’s spread out over a much larger area of paper. It’s this changing of our angle towards the Sun that gives us seasons.

The season we call ?winter? begins on the Winter Solstice. The word Solstice means ?sun still?. But to understand the significance of the Winter Solstice, we must first go back in time to the Summer Solstice, or first day of summer. Starting on June 21st, the sun gradually loses altitude in the sky as seen at noon. By September 22nd, the sun?s noon time altitude is significantly lower in the sky. The process continues until December 21st. Around this date, the sun seems to hold its position in the sky and then slowly begins to climb northward again; hence the term ?sun still.? To ancient peoples, the Solstice was a significant point in the year.

Because ancient peoples knew nothing of the earth?s tilt, the southward march of the sun was a troubling time. There was fear that one day the sun might continue moving south until was lost entirely. Many cultures conducted rituals to encourage the sun to move north again and when it did there were great celebrations. These celebrations, regardless of culture, all had a common theme that of rekindled light.

Not surprising then that many of the traditions and customs of ancient Solstice celebrations have survived to the present day. Although we know that the sun will begin moving north without any encouragement from humans, we still use this time of cold and darkness to celebrate the theme of rekindled light. From the Hanukah Menorah, to the Scandinavian Yule log, to the lights of the Christmas tree, during this season we seek to push back the darkness with light. Although the forms have evolved over the centuries, we cans still see the spirit of many of the old ways in our present day Solstice celebrations.

Now here is an interesting question to ponder, if the earth were not tilted and we had no seasons, would we celebrate the holidays in the same way?

Written by Rod Kennedy