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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 March - For this month, only Mars and Saturn put on a nice evening show. But for early risers, the morning sky provides views of Jupiter, Venus and Mercury. Cool nights in the Northern Hemisphere still provide good seeing conditions for observing the heavens this month. | |
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Mercury - Is at greatest western elongation (27°) on the 3rd. Mercury rises about 5:22 am on the 1st and about 5:21 am by month's end. Look for Mercury early in the month as Mercury rapidly descends into the early morning twilight glow before sunrise. Mercury moves from the constellation of Capricornus into Aquarius this month. Mercury shines at magnitude 0.1 on the 1st and brightens slightly to magnitude -0.1 on the 15th. |
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Venus - Rises about 5:30 am on the 1st and about 5:09 am by month's end. Look for Venus in the early morning sky before sunrise. Venus shines at magnitude -3.8 and passes from the constellation of Capricornus into Aquarius this month. |
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Earth - (US) Daylight savings time begins on the 9th. The Vernal Equinox occurs at 1:48 am EDT on the 20th. |
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Mars - Sets at 2:58 am on the 1st and about 1:43 am by month's end. Mars is in the constellation of Gemini. Look for Mars nearly overhead after sunset. Mars shines at magnitude 0.5. |
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Jupiter - Rises at 3:46 am on the 1st and about 2:01 am by month's end. Jupiter continues to climb higher in the southeast in the morning sky. Jupiter is in the constellation of Sagittarius shining at magnitude -2.0. |
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Saturn - Rises around 5:05 pm on the 1st and about 2:53 pm by month's end. Saturn is still visible for most of the evening this month. Saturn shines at magnitude 0.3 in the constellation of Leo. |
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Uranus - Is in conjunction with the Sun on the 8th and is not visible this month. |
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Neptune - Has returned to the morning sky this month but remains in the early morning twilight and will be difficult to spot. Neptune rises at 5:46 am on the 1st and about 3:47 am by month's end. Neptune is in the constellation of Capricornus shining at magnitude 8.0. |
Dwarf Planets |
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Ceres - Sets about 11:35 pm on the 1st and about 10:29 pm by month's end. Ceres is in the constellation of Taurus and shines at magnitude 8.9. |
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Pluto - Rises about 2:21 am on the 1st and about 12:20 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 - February 28, 2008 Stepping Stone to Dione Full-Res: PIA09847 "The Cassini spacecraft captures Janus in the foreground, with Dione in the distance beyond. The image was taken two hours after Hiding Dione, in which Cassini imaged Dione beyond the rings. Janus is 181 kilometers (113 miles) across. Dione is 1,126 kilometers (700 miles) across. North on the moons is up. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Jan. 17, 2008. The view was obtained at a distance of approximately 1.2 million kilometers (766,000 miles) from Janus and 1.6 million kilometers (970,000 miles) from Dione. Image scale is 7 kilometers (4 miles) per pixel on Janus and 9 kilometers (6 miles) per pixel on Dione." 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 - February 28, 2008 Memories of Jupiter "A year ago, New Horizons was flying through the heart of the Jupiter system, gradually picking up speed and systematically gathering spectacular data on the solar systemÕs largest planet and its closest moons. The results of that spectacular flyby have since been featured on thousands of electronic and printed pages, including a special issue of the journal Science in October 2007. New Horizons scientists recently took a new look at one of the more memorable images from the Jupiter collection: that of the erupting volcano Tvashtar on the moon Io. Taken through two of the four filters in the sensitive Multispectral Visible Imaging Camera, the picture shows the reddish colors of the plume deposits surrounding the base of the volcano - a view we hadnÕt seen in earlier pictures. Check it out in the New Horizons gallery." 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 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. |
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MESSENGER - February 27, 2008 Craters in Caloris "As MESSENGER sped by Mercury on January 14, 2008, the Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS) captured this image, which includes the edge of the planet against the blackness of space. Much of the foreground shows a portion of Caloris basin, one of the largest impact basins in the solar system. The two large craters near the bottom of this image can be identified on the northwestern floor of the basin on the mosaicked image of Caloris released at MESSENGERÕs NASA press conference on January 30, 2008. The large crater in the bottom middle of this image has a diameter of about 70 kilometers (40 miles)." 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 January 11, 2008 Astronomers Rule Out Possibility of Asteroid Impact on Mars "As expected, scientists at JPL's Near-Earth Object Office have further refined the trajectory estimate for asteroid 2007 WD5 and ruled out any possibility of a Mars impact on Jan. 30. The latest trajectory plot of the asteroid was made possible by adding to previously obtained data some new data from a round of observations acquired by three observatories on the evenings of Jan. 5 through 8. Based on this latest analysis, the odds for the asteroid impacting Mars on Jan. 30 are 0.0 percent. The latest observations come from the German-Spanish Astronomical Center, Calar Alto, Spain; the Multi-Mirror Telescope, Mt. Hopkins, Ariz.; and the University of Hawaii telescope, Mauna Kea, Hawaii." "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 February 18-22, 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 at: http://starbrite.jpl.nasa.gov/pds/" Visit the Mars Odyssey Mission page. |
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Mars Exploration Rover Mission (Spirit and Opportunity) - February 26, 2008
Spirit Status: Spirit Inches Downward - sol 1457-1463, February 13, 2008 "Spirit is tiptoeing ever so carefully down the north edge of the elevated volcanic plateau known as "Home Plate." Having completed a 4-centimeter (1.6-inch) drive on sol 1463 (Feb. 13, 2008), the rover's current northerly tilt is 27.1 degrees. Spirit's handlers plan to have the rover drive another 4 centimeters on sol 1464 (Feb. 14, 2008). They expect Spirit to be at the rover's final winter perch by the end of next week, following a few more 4-centimeter drives. Given recent progress, Spirit may achieve a northerly, Sun-facing tilt of 30 degrees, higher than originally anticipated. Spirit remains healthy." Opportunity Status: Opportunity Proceeds with Caution on Sandy Slopes - sol 1437-1443, Feb 14, 2008 "After recovering from a stall in Joint 1, which controls the compass orientation of the shoulder on the rover's robotic arm, Opportunity is proceeding carefully to its next target, an exposure of layered rocks known as "Gilbert." Opportunity ran the usual diagnostic tests for this sort of fault, which occurred while the rover was studying a rock target known as "Buckland," and successfully placed the Mössbauer spectrometer on the target on Sol 1437 (Feb. 8, 2008). On Sol 1438 (Feb. 9, 2008), the rover's handlers decided to relinquish further scientific studies of the target and proceed instead with a drive toward Gilbert. As this meant the rover would wander into new terrain, the team created a series of steps to allow Opportunity to characterize the surroundings along the way. One of these steps involved placing the front two wheels on an area of soil to leave a scuff on the surface and backing up to take images of the exposed area. On Sol 1438, however, prior to reaching the intended soil area, Opportunity aborted the drive. The rover completed the second planned "scuffing" on Sol 1441 (Feb. 12, 2008). This time the scuff was successful, though it revealed an interesting surprise -- Opportunity's right front wheel dug in much more than the rover's handlers had expected, highlighting the need to proceed cautiously toward Gilbert. Because Opportunity was unable to relay all of the diagnostic data to Earth at one time because the volume of data was more than could be accommodated, the rover's handlers decided that the prudent course of action was to wait one planning cycle before having Opportunity proceed with the drive. On Sol 1443 (Feb. 14, 2008), Opportunity completed a diagnostic examination of the grind bit on the rock abrasion tool and collected a mosaic of microscopic images of a rock target dubbed "Lyell Exeter," commemorating the college attended by geologist Sir Charles Lyell in the early 1800s, as well as compositional data using the alpha-particle X-ray spectrometer. Opportunity is healthy and all subsystems are performing as expected. The latest available measurements on Sol 1443 showed a power level of 469 watt-hours (100 watt-hours is the amount of energy needed to light a 100-watt bulb for 1 hour). Plans for the coming weekend called for the rover to proceed with the first of a two-step drive toward Gilbert." Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter - No new news since January 23, 2008 Orbiting Camera Details Dramatic Wind Action on Mars "Mars' atmosphere is challenging scientists to explain complex, wind-sculpted landforms seen with unprecedented detail in images from NASA's Mars Reconnaissance Orbiter. Mars has an ethereal, tenuous atmosphere with less than one-percent the surface pressure of Earth, which challenges scientists to explain complex, wind-sculpted landforms seen with unprecedented detail in images from NASA's Mars Reconnaissance Orbiter. One of the main questions has been if winds on present-day Mars are strong enough to form and change geological features, or if wind-constructed formations were made in the past, perhaps when winds speeds and atmospheric pressures were higher. The eye-opening new views of wind-driven Mars geology come from the University of Arizona's High Resolution Imaging Science Experiment camera (HiRISE). As the orbiter flies at about 3,400 meters per second (7,500 mph) between 250 and 315 kilometers (155 to 196 miles) above the Martian surface, this camera can see features as small as half a meter (20 inches)." More information about the mission is available online at http://www.nasa.gov/mro. |
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Phoenix Mars Lander Mission - February 28 - Spacecraft at Mars Prepare to Welcome New Kid on the Block
"Every landing on Mars is difficult. Having three orbiters track Phoenix as it streaks through Mars' atmosphere will set a new standard for coverage of critical events during a robotic landing. The data stream from Phoenix will be relayed to Earth throughout the spacecraft's entry, descent and landing events. If all goes well, the flow of information will continue for one minute after touchdown. "We will have diagnostic information from the top of the atmosphere to the ground that will give us insight into the landing sequence," said David Spencer of NASA's Jet Propulsion Laboratory, Pasadena, Calif., deputy project manager for the Phoenix Mars Lander project. This information would be valuable in the event of a problem with the landing and has the potential to benefit the design of future landers." 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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