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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 August - Several planets, some comets, plenty of meteors and a couple of eclipses are in store for viewers of the heavens this month. | |
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Mercury - Has returned to the evening sky this month. Mercury sets at 8:30 p.m. on the 1st and about 8:23 p.m. by month's end. Look for Mercury low in the west soon after sunset after mid-month. Mercury is in the constellation of Leo shining at magnitude -0.5. |
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Venus - Can be found low in the west soon after sunset. Venus will be the brightest object in the sky shining at magnitude -3.8. Keep an eye on Venus during the first 2 weeks of August as Venus and Saturn close in on each other. Venus sets at 8:59 p.m. on the 1st and about 08:28 p.m. by month's end. Venus is in the constellation of Leo. |
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Earth - N/A. |
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Mars - Is still visible in the evening sky after sunset. Mars sets at 9:56 p.m. on the 1st and about 8:39 p.m. by month's end. Look for Mars a little bit higher than Saturn and Mercury. Mars is in the constellation of Virgo shining at magnitude 1.7. |
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Jupiter - Is also visible in the evening sky for most of the night. Jupiter can be found in the southern sky after sunset. Jupiter sets at 4:03 a.m. on the 1st and about 1:51 a.m. by month's end. Jupiter is in the constellation of Sagittarius shining at magnitude -2.6. |
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Saturn - Is still visible in the early evening sky but just barely, not quite lost in the twilight glow during the first 2 weeks of August. Saturn sets around 9:33 p.m. on the 1st and about 7:40 p.m. by month's end. Saturn shines at magnitude 0.8 in the constellation of Leo. |
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Uranus - Rises at 9:57 p.m. on the 1st and about 7:53 p.m. by month's end. Uranus is in the constellation of Aquarius shining at magnitude 5.7. |
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Neptune - Is at opposition on the 15th. Neptune rises at 8:43 p.m. on the 1st and about 6:39 p.m. by month's end. Neptune is in the constellation of Capricornus shining at magnitude 7.8. |
Dwarf Planets |
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Ceres - Returns to the morning sky this month. Ceres rises at 3:22 a.m. on the 1st and about 2:25 a.m. by monthÕs end. Ceres is in the constellation of Gemini shining at magnitude 8.8. |
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Pluto - Sets at 3:16 a.m. on the 1st and about 1:13 a.m. by month's end. Pluto shines at magnitude 13.9 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
The 2008 Perseid Meteor Shower 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 - July 30, 2008 NASA Confirms Liquid Lake on Saturn Moon "PASADENA, Calif. -- NASA scientists have concluded that at least one of the large lakes observed on Saturn's moon Titan contains liquid hydrocarbons, and have positively identified the presence of ethane. This makes Titan the only body in our solar system beyond Earth known to have liquid on its surface. Scientists made the discovery using data from an instrument aboard the Cassini spacecraft. The instrument identified chemically different materials based on the way they absorb and reflect infrared light. Before Cassini, scientists thought Titan would have global oceans of methane, ethane and other light hydrocarbons. More than 40 close flybys of Titan by Cassini show no such global oceans exist, but hundreds of dark, lake-like features are present. Until now, it was not known whether these features were liquid or simply dark, solid material. "This is the first observation that really pins down that Titan has a surface lake filled with liquid," said Bob Brown of the University of Arizona, Tucson. Brown is the team leader of Cassini's visual and mapping instrument. The results will be published in the July 31 issue of the journal Nature." 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 - July 29, 2008 New Horizons Ventures Beyond SaturnÕs Orbit "As avid followers of New Horizons know, our spacecraft has been mostly hibernating since February, and will continue to so do until Sept. 2, when we will wake it to begin its second annual checkout. Many of you will also recall that New Horizons passed the orbit of Saturn in early June. New Horizons is the first spacecraft to venture this far (a billion kilometers from the Sun!) since the last of the Voyagers accomplished the same milestone in the summer of 1981. We are now nearly 96 million kilometers (60 million miles) beyond Saturn, and will cross the orbit of Uranus Ð about 2 billion kilometers from the Sun Ð in March 2011." 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 - July 3, 2008 MESSENGER Settles Old Debates and Makes New Discoveries at Mercury "Scientists have argued about the origins of MercuryÕs smooth plains and the source of its magnetic field for over 30 years. Now, analyses of data from the January 2008 flyby of the planet by the MESSENGER spacecraft have shown that volcanoes were involved in plains formation and suggest that its magnetic field is actively produced in the planetÕs core and is not a frozen relic. Scientists additionally took their first look at the chemical composition the planetÕs surface material. The tiny craft probed the composition of MercuryÕs thin atmosphere, sampled charged particles (ions) near the planet, and demonstrated new links between both sets of observations and materials on MercuryÕs surface. The results are reported in a series of 11 papers published in a special section of the July 4 issue of Science magazine." 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 July 21-25, 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) - July 4, 2008
Spirit Status: Biding Time - sol 1594-1600, June 27-July 03, 2008 "Spirit continues to ride out the Martian winter by doing minimal activities to conserve power. The rover conducts very light science activities every three to four Martian days, or sols, and relays data to NASA's Odyssey orbiter for transmission to Earth every 4 sols. The rest of the time, Spirit mostly sleeps. As it has been some time since Spirit's operators were able to synchronize the spacecraft clock to Earth time, they wished to determine how far the spacecraft clock had drifted (how much it had changed over time). Synchronization of the clock is a process that requires a power-intensive, two-way, X-band communications link. When the power situation allowed it, they decided to perform an X-band "beep" (a five-minute, low-gain communication session) to estimate the amount of drift. The transmission of plans to do so on sol 1594 (June 27, 2008) were not detected by the ground station. Engineers hoped to make another attempt on sol 1604 (July 7, 2008). Spirit is healthy and all subsystems were performing as expected as of the Odyssey downlink on sol 1598 (July 1, 2008). Solar-array energy has been steady within the range of 225 watt-hours to 230 watt-hours (100 watt-hours is the amount of energy needed to light a 100-watt bulb for one hour)." Opportunity Status: Rover Takes Photos of Scenic View - sol 1574-1580, June 28-July 04, 2008 "Opportunity has completed work on the stand-off portion of the full-color panorama of the layered cliff known as "Cape Verde." It may take a couple of weeks for the entire panorama to arrive on Earth, depending on the volume of data the rover is able to transmit during communications links. Next, Opportunity will move closer to Cape Verde to take a high-resolution image of a smaller area in front of the rover. During the past week, engineers characterized the performance of the rover's rock abrasion tool along the z-axis by comparing voltage and the speed of the actuator at different temperatures. In the event that the z-axis encoder lines break, as have the encoder lines for the rotate and revolve axes, this characterization will be essential in developing a functional strategy for operating the rock abrasion tool with full, open-loop control. The z-axis encoder is responsible for moving the cutting head outward into the rock. Next week's plans call for Opportunity to bump forward to a point only a few meters away from the cliff face to take high-resolution images. If possible, Opportunity will also conduct scientific studies of an outcrop target called "Nevada" (so named because of a rock next to it which has a shape reminiscent of the outline of the state of Nevada) using instruments on the robotic arm. Opportunity is healthy and all subsystems are performing as expected. Energy is around 376 watt-hours (100 watt-hours is the amount of energy required to light a 100-watt bulb for one hour). As of Sol 1578 (July 2, 2008), Tau (a measure of darkness due to atmospheric dust) was at 0.413 and the dust factor (a measure of the proportion of sunlight penetrating dust on the solar arrays) was at 0.771." Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter Mission - July 16, 2008 NASA Spacecraft Shows Diverse, Wet Environments on Ancient Mars "WASHINGTON -- Two studies based on data from NASA's Mars Reconnaissance Orbiter have revealed that the Red Planet once hosted vast lakes, flowing rivers and a variety of other wet environments that had the potential to support life. One study, published in the July 17 issue of Nature, shows that vast regions of the ancient highlands of Mars, which cover about half the planet, contain clay minerals, which can form only in the presence of water. Volcanic lavas buried the clay-rich regions during subsequent, drier periods of the planet's history, but impact craters later exposed them at thousands of locations across Mars. The data for the study derives from images taken by the Compact Reconnaissance Imaging Spectrometer for Mars, or CRISM, and other instruments on the orbiter. "The big surprise from these new results is how pervasive and long-lasting Mars' water was, and how diverse the wet environments were," said Scott Murchie, CRISM principal investigator at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md."
MARS RECONNAISSANCE ORBITER HIRISE IMAGES
More information about the MRO mission is available online. |
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Phoenix Mars Lander Mission - July 31, 2008 - NASA Spacecraft Confirms Martian Water, Mission Extended
"TUCSON, Ariz. -- Laboratory tests aboard NASA's Phoenix Mars Lander have identified water in a soil sample. The lander's robotic arm delivered the sample Wednesday to an instrument that identifies vapors produced by the heating of samples. "We have water," said William Boynton of the University of Arizona, lead scientist for the Thermal and Evolved-Gas Analyzer, or TEGA. "We've seen evidence for this water ice before in observations by the Mars Odyssey orbiter and in disappearing chunks observed by Phoenix last month, but this is the first time Martian water has been touched and tasted." With enticing results so far and the spacecraft in good shape, NASA also announced operational funding for the mission will extend through Sept. 30. The original prime mission of three months ends in late August. The mission extension adds five weeks to the 90 days of the prime mission. "Phoenix is healthy and the projections for solar power look good, so we want to take full advantage of having this resource in one of the most interesting locations on Mars," said Michael Meyer, chief scientist for the Mars Exploration Program at NASA Headquarters in Washington." 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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