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IAAS Monthly Astronomy Newsletter SUBSCRIBE Read important subscription notes below. Freelists.org |
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Background screen credits:NGC5775 -Imaged March 21/22, 2001 using the 16" Kitt Peak Visitors Center telescope as part of the Advanced Observing Program.
| Planetary Highlights for January - The new year open with Mercury and Jupiter low on the western horizon. With the cold, crisp nights of the northern hemisphere, Mercury is actually quite easy to spot along with Jupiter. Venus is high in the southwest, the brightest planetary object in the evening sky. The Moon is at its closest to the Earth this month as well. Saturn's rings have turned edge-on to us and are barely visible. Uranus and Neptune are still visible, but Mars still remains hidden. | |
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Mercury - Is at greatest eastern elongation (19° above the western horizon) on the 4th. Mercury is easily visible, low in the west soon after sunset. Look for Mercury during the first two weeks of January. Mercury is in inferior conjunction on the 20th and will not be visible after mid-month. Mercury sets at 6:13 p.m. on the 1st. Mercury is in the constellation of Sagittarius shining at magnitude -0.7. |
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Venus - Is at greatest eastern elongation (47° above the western horizon) on the 14th. Venus is in the constellation of Capricornus this month. Venus sets at 8:34 p.m. on the 1st and about 9:11 p.m. by month's end. Venus shines at magnitude -4.6. |
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Earth - Is at perihelion (91.4 million miles from the Sun) on the 4th. |
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Mars - Is still lost behind the Sun and in the twilight glow late in the month. Mars will be visible in the morning sky sometime in early February. |
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Jupiter - Can be found low on the western horizon soon after sunset. Jupiter is in conjunction with the Sun on the 24th. Jupiter will disappear in the twilight glow soon after the first week of January. Jupiter sets at 6:07 p.m. on the 1st. Jupiter is in the constellation of Sagittarius shining at magnitude -1.9. |
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Saturn - Is stationary on the 1st. Saturn rises at 10:24 p.m. on the 1st and about 8:18 p.m. by month's end. Saturn is in the constellation of Virgo shining at magnitude 0.9. |
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Uranus - Sets at 10:20 p.m. on the 1st and about 8:24 p.m. by month's end. Uranus is in the constellation of Aquarius shining at magnitude 5.9. |
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Neptune - Sets at 8:06 p.m. on the 1st and about 6:09 p.m. by month's end. Neptune is in the constellation of Capricornus shining at magnitude 8.0. |
Dwarf Planets |
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Ceres - Rises at 9:26 p.m. on the 1st and about 7:12 p.m. by monthÕs end. Ceres is in the constellation of Leo shining at magnitude 7.6. |
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Pluto -
Has returned to the morning sky rising about 6:18 a.m. on the 1st and about 4:20 a.m. by month's end. Pluto is in the constellation of Sagittarius shining at magnitude 14.1.
Good luck at spotting these two, a large telescope and dark skies will be needed. |
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Meteor Showers
For more information about Meteor Showers, visit Gary Kronk's Meteor Showers Online web page. |
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Comets
Lulin tips the scales of Libra, between ruddy Antares and blue-white Spica. Glowing at 8th magnitude, this primordial snowball hails from the distant Oort Cloud. The comet makes its closest approach to the Sun January 10, but it will continue to brighten as it approaches Earth. It's destined never to return to the inner solar system. You'll need an 8-inch telescope to spy this comet from the suburbs, but a 4-inch will reveal it under a dark sky. The second half of January belongs to 85P/Boethin. After darkness falls these cold nights, this 8th-magnitude periodic comet wades halfway up the western sky in watery Pisces. It is almost perfectly placed for evening observers. It passes 0.2 deg. north of the face-on spiral galaxy M74 the night of January 25/26. Neither object has a high surface brightness, so you'll want a dark sky to see this conjunction well. From the suburbs, only the objects' cores will be visible. You'll see their diffuse outer glows if you observe away from the city." Astronomy Magazine, January 2009, p. 54.
For more information about Comets, visit Gary Kronk's Cometography.com webpage. |
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Eclipses
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Ocultations
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Asteroids
(From west to east)
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Cassini - December 21, 2008 Titan Flyby - Dec. 21, 2008 Altimetry Over Ontario Lacus "Cassini streaked past Titan on Dec. 21 at an altitude of 971 kilometers (603 miles), obtaining radar images of Titan's south polar region and a topographic profile of the dark, possibly liquid-filled area known as Ontario Lacus." For the latest mission status reports, visit Cassini Mission Status web page. The speed and location of the spacecraft along its flight path can be viewed on the "Where is Cassini Now?" webpage. |
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New Horizons - December 19, 2008 New Horizons Earns a Holiday "After an intense annual checkout - more like a deep-space workout - New Horizons getting some well-deserved rest. New Horizons operators at the Johns Hopkins University Applied Physics Laboratory (APL) eased the spacecraft into electronic hibernation on Dec. 16, wrapping up nearly four months of tests, data collection and software upgrades. The spacecraft's Earth-bound crew has now turned its attention to detailed Pluto-encounter sequencing. "I'm in awe of all the team accomplished during this checkout - multiple software uploads, full spacecraft and payload checkouts, instrument calibrations and new capability tests, star-tracker imaging, trajectory tracking refinement, science measurements and more, and all of it went well," says New Horizons Principal Investigator Alan Stern. "What a great team and spacecraft we have!" New Horizons is spending most of its 9 1/2 -year cruise to Pluto in hibernation, with its major systems and most instruments turned off, save for an annual period when the team wakes it up for system checks and other activities. Mission managers expect each annual checkout to last about 10 weeks, but they also have to be flexible. The first annual checkout (ACO) in 2007 took about three months as operators took extra time to update the spacecraft's autonomy software and finished commissioning the science instruments." For more information on the New Horizons mission - the first mission to the ninth planet - visit the New Horizons home page. |
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Dawn - No new news since November 20, 2008 Dawn Glides Into New Year "NASA's Dawn spacecraft shut down its ion propulsion system today as scheduled. The spacecraft is now gliding toward a Mars flyby in February of next year. "Dawn has completed the thrusting it needs to use Mars for a gravity assist to help get us to Vesta," said Marc Rayman, Dawn's chief engineer, of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Dawn will now coast in its orbit around the sun for the next half a year before we again fire up the ion propulsion system to continue our journey to the asteroid belt." Dawn's ion engines may get a short workout next January to provide any final orbital adjustments prior to its encounter with the Red Planet. Ions are also scheduled to fly out of the propulsion system during some systems testing in spring. But mostly, Dawn's three ion engines will remain silent until June, when they will again speed Dawn toward its first appointment, with asteroid Vesta." For more information on the Dawn mission, visit the Dawn home page. |
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MESSENGER - December 23, 2008 MESSENGER Approaches Three Billion Miles, Enters Fourth Solar Conjunction "On December 26, the MESSENGER spacecraft will have traveled three billion miles since its launch, marking somewhat more than 60 percent of the probe's journey toward its destination to be inserted into orbit about Mercury. "That MESSENGER's odometer reading has reached another major milestone reminds us of the long and complex route that our spacecraft must follow," offers Principal Investigator Sean Solomon, of the Carnegie Institution of Washington. "The year now ending has seen the first two spacecraft flybys of the innermost planet in more than three decades, encounters that have yielded a rich lode of new observations. The journey is far from over, but MESSENGER has a skilled team to guide it the rest of the way." Mercury orbits deep within the Sun's gravity well. So, even though the planet can be as close as 82 million kilometers (51 million miles) from Earth, getting the probe into orbit around Mercury depends on an innovative trajectory using the gravity of Earth, Venus, and Mercury itself to slow and shape the probe's descent into the inner solar system. On its 4.9 billion-mile journey to becoming the first spacecraft to orbit the planet Mercury, MESSENGER has flown by Earth once, Venus twice, and Mercury twice. Still to come is one more flyby of Mercury in late September 2009. Today the spacecraft entered its fourth superior solar conjunction of the mission, placing it on the opposite side of the Sun from Earth. (To see where MESSENGER is now, visit http://messenger.jhuapl.edu/whereis/index.php.) The Sun-Earth-probe angle will be between 2° and 3° until January 6, 2009, so during the next two weeks there will be no communication with the spacecraft." For more information on the MESSENGER mission, visit the MESSENGER home page. |
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Pack Your Backpack Calling all explorers! Tour JPL with our new Virtual Field Trip site. Stops include Mission Control and the Rover Lab. Your guided tour starts when you select a ÓfaceÓ that will be yours throughout the visit. Cool space images and souvenirs are all included in your visit. |
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Past, Present, Future and Proposed JPL Missions - http://www.jpl.nasa.gov/missions Visit JPL's mission pages for current status. |
Mars Missions
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Mars Odyssey Orbiter - No new news since November 17, 2008 Gamma-Ray Evidence Suggests Ancient Mars Had Oceans "An international team of scientists who analyzed data from the Gamma Ray Spectrometer onboard NASA's Mars Odyssey reports new evidence for the controversial idea that oceans once covered about a third of ancient Mars. "We compared Gamma Ray Spectrometer data on potassium, thorium and iron above and below a shoreline believed to mark an ancient ocean that covered a third of Mars' surface, and an inner shoreline believed to mark a younger, smaller ocean," said University of Arizona planetary geologist James M. Dohm, who led the international investigation. "Our investigation posed the question, Might we see a greater concentration of these elements within the ancient shorelines because water and rock containing the elements moved from the highlands to the lowlands, where they eventually ponded as large water bodies?" Dohm said." "A simulated fly-through using the newly assembled imagery is available online. The fly-through plus tools for wandering across and zooming into the large image are at THEMIS."
Mars Odyssey THEMIS Images December 24-31, 2008 The following new images from the Mars Odyssey spacecraft are now available:
The Odyssey data are available through a new online access system established by the Planetary Data System. Visit the Mars Odyssey Mission page. |
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Mars Exploration Rover Mission (Spirit and Opportunity) - December 29
Mars Rovers Near Five Years of Science and Discovery "PASADENA, Calif. -- NASA rovers Spirit and Opportunity may still have big achievements ahead as they approach the fifth anniversaries of their memorable landings on Mars. Of the hundreds of engineers and scientists who cheered at NASA's Jet Propulsion Laboratory in Pasadena, Calif., on Jan. 3, 2004, when Spirit landed safely, and 21 days later when Opportunity followed suit, none predicted the team would still be operating both rovers in 2009. "The American taxpayer was told three months for each rover was the prime mission plan," said Ed Weiler, associate administrator for NASA's Science Mission Directorate at NASA Headquarters in Washington. "The twins have worked almost 20 times that long. That's an extraordinary return of investment in these challenging budgetary times." The rovers have made important discoveries about wet and violent environments on ancient Mars. They also have returned a quarter-million images, driven more than 21 kilometers (13 miles), climbed a mountain, descended into craters, struggled with sand traps and aging hardware, survived dust storms, and relayed more than 36 gigabytes of data via NASA's Mars Odyssey orbiter. To date, the rovers remain operational for new campaigns the team has planned for them." Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter Mission - December 18, 2008 Scientists Find 'Missing' Mineral and Clues to Mars Mysteries "Surveying intact bedrock layers with the Compact Reconnaissance Imaging Spectrometer for Mars, or CRISM, scientists found carbonate minerals, indicating that Mars had neutral to alkaline water when the minerals formed at these locations more than 3.6 billion years ago. Carbonates, which on Earth include limestone and chalk, dissolve quickly in acid. Therefore, their survival until today on Mars challenges suggestions that an exclusively acidic environment later dominated the planet. Instead, it indicates that different types of watery environments existed. The greater the variety of wet environments, the greater the chances one or more of them may have supported life. "We're excited to have finally found carbonate minerals because they provide more detail about conditions during specific periods of Mars' history," said Scott Murchie, principal investigator for the instrument at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md. The findings will appear in the Dec. 19 issue of Science magazine and were announced Thursday at a briefing at the American Geophysical Union's Fall Meeting in San Francisco."
MARS RECONNAISSANCE ORBITER HIRISE IMAGES
More information about the MRO mission is available online. |
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Phoenix Mars Lander Mission - December 15, 2008 Phoenix Site on Mars May Be in Dry Climate Cycle Phase "PASADENA, Calif. -- The Martian arctic soil that NASA's Phoenix Mars Lander dug into this year is very cold and very dry. However, when long-term climate cycles make the site warmer, the soil may get moist enough to modify the chemistry, producing effects that persist through the colder times. Phoenix found clues increasing scientists' confidence in predictive models about water vapor moving through the soil between the atmosphere and subsurface water-ice. The models predict the vapor flow can wet the soil when the tilt of Mars' axis, the obliquity, is greater than it is now. The robot worked on Mars for three months of prime mission, plus two months of overtime, after landing on May 25. The Phoenix science team will be analyzing data and running comparison experiments for months to come. With some key questions still open, team members at a meeting of the American Geophysical Union today reported on their progress. "We have snowfall from the clouds and frost at the surface, with ice just a few inches below, and dry soil in between," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson. "During a warmer climate several million years ago, the ice would have been deeper, but frost on the surface could have melted and wet the soil." With no large moon like Earth's to stabilize it, Mars goes through known periodic cycles when its tilt becomes much greater than Earth's. During those high-tilt periods, the sun rises higher in the sky above the Martian poles than it does now, and the arctic plain where Phoenix worked experiences warmer summers." Visit the Phoenix Mars Lander Mission pages. |
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Mars Missions Status
New Mars missions are being planned to include several new rover and sample collection missions. Check out the Mars Missions web page and the Mars Exploration page. |

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