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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 - "This January is a great month for stargazing. Mars is near its best. Jupiter and Venus perform a spectacular morning conjunction. Comet 8P/Tuttle is on view early in the month. And the prolific Quadrantid meteor shower occurs with little lunar interference. Throw in the Moon's occultation of the Pleiades star cluster, and the only thing that could improve observing would be warmer temperatures. All in all, it's not a bad way to start off the year." Astronomy Magazine, January 2008, p. 44. | |
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Mercury - Is at greatest eastern elongation (19° above the western horizon) on the 21st and is stationary on the 28th. Mercury is visible most of the month in the western sky after sunset. Mercury sets about 5:19 pm on the 1st and about 6:12 pm by month's end. Mercury moves from the constellation of Sagittarius, through Capricornus, into Aquarius this month and dims from magnitude -1.0 to 1.4. |
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Venus - Rises about 4:21 am on the 1st and about 5:15 am by month's end. Venus shines at magnitude -3.9 and passes from the constellation of Libra into Sagittarius this month. |
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Earth - Is at perihelion (91.4 million miles from the Sun) on the 2nd. |
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Mars - Having reached opposition last month, Mars still remains a prime telescopic treat. Mars is well above the eastern horizon (about 30° or more) as the Sun sets. Mars rises at 3:30 pm on the 1st and about 1:05 pm by month's end. Mars is in the constellation of Taurus and shines at magnitude -1.5. |
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Jupiter - Will be difficult to spot early in the month as Jupiter rises just 20 minutes before the Sun on the 1st. Wait until mid-month for better viewing. Jupiter rises at 6:52 am on the 1st and about 5:18 am by month's end. Jupiter is very low in the southeast in the constellation of Sagittarius shining at magnitude -1.8. |
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Saturn - Rises around 9:21 pm on the 1st and about 7:11 pm by month's end. Saturn reaches opposition next month so Saturn is in an excellent position for evening viewing. Saturn shines at magnitude 0.5 in the constellation of Leo. |
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Uranus - Sets about 10:42 pm on the 1st and about 8:08 pm by month's end. Uranus is in the constellation of Aquarius and shines at a magnitude of 5.9. |
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Neptune - Sets at 9:56 pm on the 1st and about 7:58 pm by month's end. Neptune is in the constellation of Capricornus and shines at magnitude 7.9. |
Dwarf Planets |
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Ceres - Sets about 2:34 am on the 1st and about 12:54 am by month's end. Ceres should be easy to spot with a small telescope this month. Ceres moves from the constellation of Cetus into Aries and shines at magnitude 8.2. |
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Pluto - Has returned to the morning sky this month. Pluto rises about 6:10 am on the 1st and about 4:12 am by month's end. Pluto shines at magnitude 14.0 in the constellation of Sagittarius. As always, good luck at spotting this one, a large telescope and very 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
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 24, 2007 - The Painted Globe Full-Res: PIA08396 "Saturn in the Cassini era has proved to be an unexpectedly colorful place, compared to the browns and golds imaged by the two Voyager spacecraft. Saturn is headed toward equinox in 2009, followed by springtime in the northern hemisphere. Having a spacecraft in orbit while such changes occur will be of great benefit in scientists' quest to understand the atmospheres of the giant planets. The planet's oblate, or squashed, shape is clearly visible in this view. The low-density planet rotates so fast (in about 10.5 hours) that it flattens out slightly around its middle. The bluish tint of the northern latitudes is presumed to be a seasonal effect, and will likely disappear entirely as the north receives increasingly greater amounts of sunlight." For the latest mission status reports, visit Cassini Mission Status webpage. 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 11, 2007 - New Horizons Team to Talk Jupiter Science at AGU Fall Meeting
"The New Horizons spacecraft's spectacular flight past Jupiter earlier this year -- which gave it a gravitational boost on the way to a 2015 encounter with Pluto -- also provided an opportunity to test the instruments on the NASA probe while gathering new scientific data. Members of the New Horizons team will present findings from that encounter during the American Geophysical Union (AGU) Fall Meeting this week in San Francisco. A combination of technology, trajectory and good timing allowed New Horizons to explore details that no spacecraft had seen before, such as lightning near Jupiter's poles, the life cycle of fresh ammonia clouds in Jupiter's atmosphere, the structure inside volcanic eruptions on Jupiter's planet-sized moon Io, and the path of charged particles traversing the previously unexplored length of Jupiter's long magnetic tail." For more information on the New Horizons mission - the first mission to the ninth planet - visit the New Horizons homepage: http://pluto.jhuapl.edu/ for more information about the mission. |
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Dawn - December 18, 2007 - NASA's Dawn Spacecraft Begins Interplanetary Cruise Phase
"NASA's Dawn spacecraft has successfully completed the initial checkout phase of the mission and begun its interplanetary cruise phase, which is highlighted by nearly continuous thrusting of its ion propulsion system. Dawn is on a 8-year, 3-billion mile journey to asteroid Vesta and dwarf planet Ceres." For more information on the Dawn mission, visit the Dawn home page for more information about the mission. |
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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 Global Surveyor
Every six months, a new suite of MGS MOC data are archived with the NASA Planetary Data System (PDS). Information about how to submit requests is online at the new Mars Orbiter Camera Target Request Site, at http://www.msss.com/plan/intro" Newly-released MOC images can be seen in the MOC Gallery, a website maintained by Malin Space Science Systems, the company that built and operates MOC for the Jet Propulsion Laboratory and NASA. Visit the MGS pages at http://mars.jpl.nasa.gov/mgs/index.html. There are over 200,000 images of Mars from the MGS, check out the newest MGS images of the surface of Mars. |
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Mars Odyssey Orbiter - December 20, 2007 - Mars Opposition
Artist's concept of Mars Opposition on December 24, 2007. The distances between the sun, the planets, and the distant nebula are not to scale. "Like all the planets in our solar system, Earth and Mars orbit the sun. But Earth is closer to the sun, and therefore races along its orbit more quickly. Earth makes two trips around the sun in about the same amount of time that Mars takes to make one trip. So sometimes the two planets are on opposite sides of the sun, very far apart, and other times, Earth catches up with its neighbor and passes relatively close to it." "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 http://themis.asu.edu."
Mars Odyssey THEMIS Images December 24-28, 2007 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 at: http://starbrite.jpl.nasa.gov/pds/" Visit the Mars Odyssey Mission page. |
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Mars Exploration Rover Mission (Spirit and Opportunity) - December 26, 2007
Spirit Status: Spirit Makes It to a North-Facing Slope - sol 1404-1408, December 21, 2007 "Spirit has achieved 13 degrees of northerly tilt after backing the rear and middle wheels over the north edge of "Home Plate," where the rover will remain during the coming holidays. Power levels have already increased significantly from 260 watt-hours on sol 1404 (Dec. 15, 2007) to 291 watt-hours on sol 1408 (Dec. 19, 2007). Spirit's ideal northerly tilt at present would be 16 degrees, and the rover's handlers plan to have the rover creep farther down the slope in mid-January to increase the northerly tilt. On Spirit's current track, they expect to see an ultimate northerly tilt of 25 degrees to 30 degrees. In the meantime, Spirit will perform studies using instruments on the rover's robotic arm, including the microscopic imager, alpha-particle X-ray spectrometer, and Mössbauer spectrometer. Spirit's handlers still have a huge challenge ahead, but after three weeks of working on Mars time and on weekends, they are, like the rover, enjoying a long-awaited and well-deserved sigh of relief. The science team is nicknaming features in the area after the Tuskegee Airmen, the first black pilots to serve in the U.S. military." Opportunity Status: Opportunity Maneuvers Around Steeper Slopes in "Victoria Crater" - sol 1375-1381, Dec 17, 2007 "Opportunity is now in the process of driving to the third band of light-colored rocks that circumscribe "Victoria Crater" beneath the rim. Scientists had initially planned to have the rover head directly downhill to a rock target nicknamed "Ronov," within the band known as "Lyell." They selected an alternate rock exposure, dubbed "Newell," when engineers determined that the original drive route would tilt the rover 25 degrees, somewhat higher than desired. The estimated tilt along the new route is a much gentler 20 degrees but the drive is somewhat more complex and required two days of planning. During the past week, Opportunity completed scientific investigation of the second band of rocks, known as "Smith," with an analysis of elemental chemistry and iron-bearing minerals beneath the surface of a rock exposure labeled "Smith2." To do this, the rover collected data with the alpha-particle X-ray spectrometer Mössbauer spectrometer, respectively. If next week's planned drive goes as anticipated and closer inspection of Newell deems it to be an acceptable target, Opportunity is likely to stay at the new location for several weeks collecting data. Scientists plan to have the rover conduct a complete campaign of studies with the alpha-particle X-ray and Mössbauer spectrometers, microscopic imager, rock abrasion tool, and on-board cameras. During the planned drive, Opportunity will complete a "Get Quick Fine Attitude," a procedure for determining the rover's position relative to the changing position of the Sun. This activity recalibrates the inertial measurement unit and eliminates tiny errors that accumulate over time in pointing the antenna. Opportunity is healthy and all subsystems are operating as expected. The latest available power readings, taken on Martian day, or sol, 1379 (Dec. 10, 2007), show solar energy levels at a robust 601 watt-hours, enough to light a 100-watt bulb for 6 hours." Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter - December 11, 2007 - Mars Orbiter Examines 'Lace' and 'Lizard Skin' Terrain
Dark fans and bright fans on Mars "SAN FRANCISCO - Scrutiny by NASA's newest Mars orbiter is helping scientists learn the stories of some of the weirdest landscapes on Mars, as well as more familiar-looking parts of the Red Planet. One type of landscape near Mars' south pole is called "cryptic terrain" because it once defied explanation, but new observations bolster and refine recent interpretations of how springtime outbursts of carbon-dioxide gas there sculpt intricate patterns and paint seasonal splotches. "A lot of Mars looks like Utah, but this is an area that looks nothing like Planet Earth," said Candice Hansen of NASA's Jet Propulsion Laboratory, Pasadena, Calif., deputy principal investigator for the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter." More information about the mission is available online at http://www.nasa.gov/mro. |
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Phoenix Mars Lander Mission - No new news since October 30, 2007 - Phoenix Mars Lander Status Report: Tasks En Route to Mars Include Course Tweak, Gear Checks
"NASA's Phoenix Mars Lander, launched on Aug. 4 and headed to Mars, fired its four trajectory correction thrusters Wednesday for only the second time. The 45.9-second burn nudged the spacecraft just the right amount to put it on a course to arrive at the red planet seven months from today. At Mars, Phoenix will face a challenging 7-minute descent through the atmosphere to land in the far north on May 25, 2008. After landing, it will use a robotic digging arm and other instruments during a three-month period to investigate whether icy soil of the Martian arctic could have ever been a favorable environment for microbial life. The solar-powered lander will also look for clues about the history of the water in the ice and will monitor weather as northern Mars' summer progresses toward fall." 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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