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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 - For the first month of the new year, seven planets grace the evening and morning skies. Venus and Jupiter are visible in the early evening before sunset. Uranus and Neptune are also visible in the evening, though observers will need binoculars or a small telescope to see these two. Mars appears in the late evening growing brighter as it approaches opposition in March. Saturn is visible in the early morning skies. Mercury makes a brief appearance before sunrise during the first week of January. The Quadrantids meteor shower should put on a respectable show as well. | |
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Mercury - Rises at 5:53 a.m. on the 1st and about 7:07 a.m. by month's end. Look for Mercury low on the eastern horizon about 30 minutes before sunrise during the first week of the month. Mercury moves from the constellation of Ophiuchus into Capricornus shining at magnitude -0.4. |
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Venus -
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Earth - Is at perihelion (91.4 million miles from the Sun) on the 4th. |
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Mars -
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Jupiter -
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Saturn - Rises at 1:33 a.m. on the 1st and about 11:33 p.m. by month's end. Saturn is visible in the morning sky before sunrise. Saturn is in the constellation of Virgo shining at magnitude 0.7. |
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Uranus - Sets at 11:21 p.m. on the 1st and about 9:24 p.m. by month's end. Look to the southwest soon after sunset to spot Uranus. Binoculars or a small telescope may be needed. Uranus is in the constellation of Pisces shining at magnitude 5.9. |
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Neptune -
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Dwarf Planets |
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Ceres - Sets at 10:38 p.m. on the 1st and about 9:25 p.m. by month's end. Ceres moves from the constellation of Aquarius into Cetus shining at magnitude 8.9. |
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Pluto -
Was in conjunction with the Sun on December 29th. Pluto will return to the morning sky during the last two weeks of the month. Pluto rises about 4:55 a.m. by month's end. Pluto is still difficult to view. Pluto is in the constellation of Sagittarius shining at magnitude 14.1.
As always, good luck at spotting these two, a large telescope and dark skies will be needed. |
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Meteor Showers
This year, the Quadrantids may prove to be quite active. See http://astronomy.com/en/News-Observing/News/2011/12/2012%20Quadrantids.aspx. 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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Observational Opportunities
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Asteroids
(From west to east)
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Ocultations
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Cassini - January 02, 2012 Titan Flyby (T-80): A Southern Swing High Over Titan "On this high-altitude encounter of Titan, the imaging science subsystem (ISS) will perform high-resolution observations around closest-approach along the anti-Saturnian and trailing hemispheres at mid- to high southern latitudes. This is one of ISS' so-called "10-pointer" flybys, i.e. one of the two scientifically most significant Titan fly-bys for ISS during the Solstice mission. As the lead instrument on the inbound approach to Titan, the composite infrared spectrometer (CIRS) instrument views Titan at various distances and spectral resolutions to make maps of atmospheric and surface temperature. After closest approach, RADAR will do radiometry of the sub-Saturn hemisphere. Outbound, the visible and infrared mapping spectrometer (VIMS) will perform stellar occultations of the stars CW Leo and R Leo, which will constrain the composition and the spectral properties of Titan's atmosphere. During the flyby, the radio and plasma wave science (RPWS) will measure thermal plasmas in Titan's ionosphere and surrounding environment, search for lightning in Titan's atmosphere, and investigate the interaction of Titan with Saturn's magnetosphere." 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 20, 2011 SwRI researchers discover new evidence for complex molecules on Pluto's surface "Boulder, Colo. - Dec. 20, 2011 - The new and highly sensitive Cosmic Origins Spectrograph aboard the Hubble Space Telescope has discovered a strong ultraviolet-wavelength absorber on Pluto's surface, providing new evidence that points to the possibility of complex hydrocarbon and/or nitrile molecules lying on the surface, according to a paper recently published in the Astronomical Journal by researchers from Southwest Research Institute and Nebraska Wesleyan University. Such chemical species can be produced by the interaction of sunlight or cosmic rays with Pluto's known surface ices, including methane, carbon monoxide and nitrogen." Find New Horizons in the iTunes App Store here. 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 - December 21, 2011 Dawn Obtains First Low Altitude Images of Vesta "PASADENA, Calif. - NASA's Dawn spacecraft has sent back the first images of the giant asteroid Vesta from its low-altitude mapping orbit. The images, obtained by the framing camera, show the stippled and lumpy surface in detail never seen before, piquing the curiosity of scientists who are studying Vesta for clues about the solar system's early history. At this detailed resolution, the surface shows abundant small craters, and textures such as small grooves and lineaments that are reminiscent of the structures seen in low-resolution data from the higher-altitude orbits. Also, this fine scale highlights small outcrops of bright and dark material. A gallery of images can be found online at: http://www.nasa.gov/mission_pages/dawn/multimedia/gallery-index.html." For more information on the Dawn mission, visit the Dawn home page. |
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MESSENGER - December 22, 2011 A Christmas Crater on Mercury "The crater at the center of Wednesday's MESSENGER image of the day is named Dickens, after Charles Dickens, the English novelist who lived from 1812 to 1870. Among Dickens' most famous works is A Christmas Carol, the story of miserly Ebenezer Scrooge and his tortured journey to a more humanitarian and generous nature. This image was acquired as part of the Mercury Dual Imaging System's (MDIS) high-resolution surface morphology base map. The surface morphology base map will cover more than 90% of Mercury's surface with an average resolution of 250 meters per pixel (0.16 miles per pixel). Images acquired for the surface morphology base map typically have off-vertical Sun angles (i.e., high incidence angles) and visible shadows so as to reveal clearly the topographic form of geologic features. Since entering orbit around Mercury on March 18, 2011, the MDIS has beamed back more than 70,000 images of the surface of the planet. The mission's imaging team has been releasing at least one new image every weekday. They are available online at http://messenger.jhuapl.edu/gallery/sciencePhotos/. During the one-year primary mission, MDIS is scheduled to acquire more than 75,000 images in support of MESSENGER's science goals." 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 "face" 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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JMARS JMARS is an acronym that stands for Java Mission-planning and Analysis for Remote Sensing. It is a geospatial information system (GIS) developed by ASU's Mars Space Flight Facility to provide mission planning and data-analysis tools to NASA's orbiters, instrument team members, students of all ages, and the general public. |
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Mars Science Laboratory - December 13, 2011 NASA Mars-Bound Rover Begins Research In Space "PASADENA, Calif. -- NASA's car-sized Curiosity rover has begun monitoring space radiation during its 8-month trip from Earth to Mars. The research will aid in planning for future human missions to the Red Planet. Curiosity launched on Nov. 26 from Cape Canaveral, Fla., aboard the Mars Science Laboratory. The rover carries an instrument called the Radiation Assessment Detector (RAD) that monitors high-energy atomic and subatomic particles from the sun, distant supernovas and other sources. These particles constitute radiation that could be harmful to any microbes or astronauts in space or on Mars. The rover also will monitor radiation on the surface of Mars after its August 2012 landing. "RAD is serving as a proxy for an astronaut inside a spacecraft on the way to Mars," said Don Hassler, RAD's principal investigator from the Southwest Research Institute in Boulder, Colo. "The instrument is deep inside the spacecraft, the way an astronaut would be. Understanding the effects of the spacecraft on the radiation field will be valuable in designing craft for astronauts to travel to Mars." Previous monitoring of energetic-particle radiation in space has used instruments at or near the surface of various spacecraft. The RAD instrument is on the rover inside the spacecraft and shielded by other components of Mars Science Laboratory, including the aeroshell that will protect the rover during descent through the upper atmosphere of Mars." Visit the Mars Science Laboratory page. |
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Mars Exploration Rover Mission (Spirit and Opportunity) - December 27, 2011
SPIRIT UPDATE: Spirit Remains Silent at Troy - sols 2621-2627, May 18-24, 2011: "No communication has been received from Spirit since Sol 2210 (March 22, 2010). More than 1,300 commands were radiated to Spirit as part of the recovery effort in an attempt to elicit a response from the rover. No communication has been received from Spirit since Sol 2210 (March 22, 2010). The project concluded the Spirit recovery efforts on May 25, 2011. The remaining, pre-sequenced ultra-high frequency (UHF) relay passes scheduled for Spirit on board the Odyssey orbiter will complete on June 8, 2011. Total odometry is unchanged at 7,730.50 meters (4.80 miles)." OPPORTUNITY UPDATE: Positioned at Candidate Site for Winter - sols 2813-2817, December 23-27, 2011: "Opportunity is positioned at a candidate site for Mars' southern hemisphere winter. The rover is at the north end of 'Cape York' on the rim of Endeavour Crater, tilted about 15 degrees to the north for favorable solar energy production. Opportunity experienced anomalously high current in the right-front wheel on Sol 2808 (Dec. 17, 2011). Diagnostics on Sols 2810 and 2812 (Dec. 20 and 22, 2011) indicated a nominal wheel and drive actuator with the terrain being the indicated explanation for the high current. On Sol 2816 (Dec. 26, 2011), the rover performed an 8-inch (0.2-meter) diagnostic backward drive. The drive completed successfully with Opportunity maintaining its 15-degree northerly tilt, sufficient for the winter period. The plan ahead is to conduct some contact measurements with the instruments on the robotic arm to see if this location offers substantive in-situ science opportunities during the winter months. Opportunity will also begin a radio Doppler tracking campaign at the start of the new year. As of Sol 2817 (Dec. 27, 2011), solar array energy production was 290 watt-hours with an atmospheric opacity (Tau) of 0.685 and a solar array dust factor of 0.475. Total odometry as of Sol 2816 (Dec. 26, 2011) is 21.35 miles (34,361.37 meters)." Visit the Mars Exploration Rover page. |
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Mars Reconnaissance Orbiter Mission - November 17, 2011 New Tool for Touring Mars Using Detailed Images "An improved tool debuts today for viewing channels, dunes, boulders and other features revealed in the huge image files from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. The new tool, HiView, offers the best way to take a personal, virtual hike through any of thousands of square miles of Mars observed by HiRISE, seeing details as small as a desk. To watch the tutorial video and download the free HiView application, go to: http://www.uahirise.org/hiview/."
MARS RECONNAISSANCE ORBITER HIRISE IMAGES More information about the MRO mission is available online. |
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Mars Odyssey Orbiter
"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."
Daily Mars Odyssey THEMIS Images 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 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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