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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 October - Planetary treats abound this month. Venus and Jupiter are visible in the early evening, Uranus and Neptune follow in mid-evening. Saturn and Mercury can be spotted before sunrise. The Orionid meteor shower also peaks later in the month. | |
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Mercury - Is at inferior conjunction with the Sun on the 6th. Mercury is at greatest western elongation (18° above the eastern horizon) on the 22nd. Mercury is at its best predawn view for this year. Look for Mercury low in the east just before sunrise later in the month. Mercury rises about 5:56 a.m. on the 15th and about 6:29 a.m. by month's end. Mercury is in the constellation of Virgo shining at magnitude 0.9 on the 15th, brightening to magnitude -0.9 on the 31st. |
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Venus - Can be found low in the West soon after sunset. Venus sets at 7:56 p.m. on the 1st and about 6:51 p.m. by month's end. Venus moves through the constellation of Libra into Scorpio this month. Mercury shines at magnitude -3.9. |
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Earth - N/A. |
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Mars - Is still visible in the evening sky after sunset but just barely. About your only chance this month will be on the 1st but you'll need a low, clear, flat western horizon. Mars will still be difficult to spot through the evening twilight haze. Mars will disappear for the next several months. Mars sets at 7:28 p.m. on the 1st. Mars is in the constellation of Virgo shining at magnitude 1.6. |
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Jupiter - Can be found in the southwestern sky soon after sunset. Jupiter sets at 11:53 p.m. on the 1st and about 9:08 p.m. by month's end. Jupiter is in the constellation of Sagittarius shining at magnitude -2.2. |
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Saturn - Rises at 4:59 a.m. on the 1st and about 2:13 a.m. by month's end. Saturn is in the constellation of Leo shining at magnitude 1.0. |
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Uranus - Sets at 5:29 a.m. on the 1st and about 2:22 a.m. by month's end. Uranus is in the constellation of Aquarius shining at magnitude 5.8. |
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Neptune - Sets at 3:08 a.m. on the 1st and about 12:04 a.m. by month's end. Neptune is in the constellation of Capricornus shining at magnitude 7.9. |
Dwarf Planets |
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Ceres - Rises at 1:29 a.m. on the 1st and about 12:24 a.m. by monthÕs end. Ceres is in the constellation of Leo shining at magnitude 8.6. |
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Pluto - Sets at 11:11 p.m. on the 1st and about 8:11 p.m. 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 - September 30, 2008 Saturn's Active Atmosphere Full-Res: PIA10480 "Saturn's high north is a seething cauldron of activity filled with roiling cloud bands and swirling vortices. A corner of the North Polar Hexagon is seen at upper left. This view looks toward a region located about 70 degrees north of the planet's equator, in a place that receives continually increasing amounts of sunlight as Saturn's seasons change. The image was taken with the Cassini spacecraft wide-angle camera on Aug. 25, 2008 using a spectral filter sensitive to wavelengths of infrared light centered at 752 nanometers. The view was obtained at a distance of approximately 541,000 kilometers (336,000 miles) from Saturn. Image scale is 29 kilometers (18 miles) per pixel." 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 - September 16, 2008 NASA Salutes New Horizons Team "The New Horizons team Ð including hundreds of technicians, engineers, scientists, managers, educators and communications specialists from more than 20 institutions across the country Ð has been given the NASA Group Achievement Award for creating and launching the first mission to Pluto and the Kuiper Belt. NASA Planetary Science Division Director James Green made the presentation Sept. 11 at the Johns Hopkins Applied Physics Lab in Laurel, Md., where New Horizons was designed and built, and is now operated. APL also manages the mission for NASAÕs Science Mission Directorate; John Sommerer, acting head of the LabÕs Space Department, accepted the award on behalf of the many APL staff members who developed the mission and spacecraft." 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 - September 29, 2008 MLA Ready to Range to MercuryÕs Surface "One week from today, the MESSENGER spacecraft will fly by Mercury for the second time this year. As part of the final preparations for this encounter, the Mercury Laser Altimeter (MLA) has been powered on after having been off since shortly after the first flyby at the beginning of the year. The entire MESSENGER science payload is now powered and configured to collect data during next weekÕs encounter. ÒRight after the January flyby, the MLA completed passive observations of Mercury, without the laser firing, as a calibration,Ó explained MLA Instrument Scientist Olivier Barnouin-Jha of the Johns Hopkins University Applied Physics Laboratory in Laurel, Md. ÒAt that point it was switched off, and it has remained off since that time.Ó During MESSENGERÕs first Mercury encounter, the MLA provided the first direct measurements of the topography of Mercury from spacecraft. The results provide evidence for a complex geologic history and indicate that MercuryÕs craters are shallower than those on the Moon at a given crater diameter, as expected because of the higher surface gravity. ÒUnlike the topographic data obtained during the first flyby, which were of terrain for which we have no space-based imaging, some of the area to which MLA will range during this second encounter was imaged by the Mercury Dual Imaging System (MDIS) during the first Mercury flyby,Ó Barnouin-Jha said. Moreover, terrain sampled by MLA during the first flyby will in turn be imaged by MDIS during this visit. ÒSo this second flyby will allow the first inter-comparison between the topographic observations and high-resolution spacecraft images,Ó he added." 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 March 20, 2008 NASA Mission Finds New Clues to Guide Search for Life on Mars "PASADENA, Calif. - NASA's Mars Odyssey orbiter has found evidence of salt deposits. These deposits point to places where water once was abundant and where evidence might exist of possible Martian life from the Red Planet's past. A team led by Mikki Osterloo of the University of Hawaii, Honolulu, found approximately 200 places on southern Mars that show spectral characteristics consistent with chloride minerals. Chloride is part of many types of salt, such as sodium chloride or table salt. The sites range from about a square kilometer (0.4 square mile) to 25 times that size." "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 September 22-26, 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) - September 20, 2008
Spirit Status: Warming Up on Mars - sol 1669-1677, September 12-20, 2008 "With Martian winter on the wane, Spirit is using significantly less energy to stay warm. During the winter solstice, Spirit needed 90 watt-hours to run the heater. Now, the rover uses between 30 and 40 watt-hours. The reduced demand for power, more than the slow increase in solar-array input, has freed up energy for other things. In particular, Spirit has added more images to the 360-degree view of its winter surroundings, known as the "Bonestell panorama." The top tier, one of three tiers needed for the final image mosaic, is almost complete. Plans called for Spirit to use the miniature thermal emission spectrometer for the first time in several months. The last time the rover used the instrument was on Martian day, or sol, 1558 (May 21, 2008). On sol 1675 (Sept. 18, 2008), Spirit's schedule of activities included calibrating the spectometer and using it to observe the sky and ground. Normally, scientists use the observations to measure temperatures at different heights and create a temperature profile of the ground and atmosphere. In this case, the purpose of the measurements is to verify that the spectrometer is still working after a long, cold period of disuse. The measurements will also enable scientists to estimate the amount of dust on the optics. They may or may not provide a useful temperature profile. Spirit is healthy and all subsystems are performing as expected as of the most recent report from NASA's Odyssey orbiter on sol 1674 (Sept. 17, 2008). Solar-array energy has inched upward to 255 watt-hours (100 watt-hours is the amount of energy needed to light a 100-watt bulb for one hour). Skies are clearer than last week, with tau, a measure of the amount of sunlight blocked by atmospheric dust, dropping to 0.141." Opportunity Status: Slipping Like a Dune Buggy - sol 1648-1654, September 12-18, 2008 "During the past week, Opportunity has been trying to reach a patch of dust between two crests of the ridge surrounding "Victoria Crater." The rover approached the ridge from the west, driving on flat ground, on Martian days, or sols, 1648 and 1650 (Sept. 12 and Sept. 14, 2008). Then, after reaching a staging position, Opportunity began to climb the ridge. That's when the rover's wheels began slipping excessively on the sandy slope. Rover drivers decided to give Opportunity another chance to make it up the slope by loosening the slip constraints. This allowed Opportunity to keep trying to climb the slope with a higher rate of wheel slippage. If the attempt to do this as planned on sol 1654 (Sept. 18, 2008) is not successful, rover drivers may try a different approach or abandon the effort. After the dust patch campaign, plans call for Opportunity to drive south toward a 20-kilometer-wide (12-mile-wide) crater 12 kilometers (7.5 miles) away. Opportunity is healthy, and all subsystems are performing as expected. Based on the latest data from sol 1653 (Sept. 17, 2008), the rover has 582 watt-hours of solar power available each day. (One hundred watt-hours is the amount of energy needed to light a 100-watt bulb for one hour.)" Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter Mission - September 25, 2008 NASA Orbiter Reveals Rock Fracture Plumbing on Mars "PASADENA, Calif. Ð NASA's Mars Reconnaissance Orbiter has revealed hundreds of small fractures exposed on the Martian surface that billions of years ago directed flows of water through underground Martian sandstone. Researchers used images from the spacecraft's High Resolution Imaging Science Experiment, or HiRISE, camera. Images of layered rock deposits at equatorial Martian sites show the clusters of fractures to be a type called deformation bands, caused by stresses below the surface in granular or porous bedrock. "Groundwater often flows along fractures such as these, and knowing that these are deformation bands helps us understand how the underground plumbing may have worked within these layered deposits," said Chris Okubo of the U.S. Geological Survey in Flagstaff, Ariz."
MARS RECONNAISSANCE ORBITER HIRISE IMAGES
More information about the MRO mission is available online. |
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Phoenix Mars Lander Mission - September 29, 2008 - NASA Mars Lander Sees Falling Snow, Soil Data Suggest Liquid Past
"PASADENA, Calif. -- NASA's Phoenix Mars Lander has detected snow falling from Martian clouds. Spacecraft soil experiments also have provided evidence of past interaction between minerals and liquid water, processes that occur on Earth. A laser instrument designed to gather knowledge of how the atmosphere and surface interact on Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing site. Data show the snow vaporizing before reaching the ground. "Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University, Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be looking for signs that the snow may even reach the ground.'" 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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