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Excerpts from JPL mission updates are provided as a public service as part
Background screen credits: NGC5775 - Imaged March 21/22, 2001 using the 16" Kitt Peak Visitors Center telescope as part of the Advanced Observing Program.
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|Planetary Highlights for March - Jupiter continues to dominate the evening skies this month and is still prominent until the early hours of the morning. Venus reaches its farthest point away from the Sun and Mercury reaches its highest point above the horizon in the morning sky. Mars, Ceres and Saturn are all visible in the late evening and early morning sky. Uranus can be spotted in the early evening and Neptune has returned to the morning sky this month.|
|Mercury - Is at greatest western elongation (28° above the eastern horizon) on the 14th. Mercury is visible, low on the eastern horizon about 30 minutes before sunrise for the month of March. Mercury rises about 5:27 a.m. on the 1st and about 6:05 a.m. by month's end. Mercury is in the constellation of Aquarius shining at magnitude 0.1 on the 15th.|
|Venus - Venus rises about 4:07 a.m. on the 1st and about 4:48 a.m. by month's end. Venus appears at its farthest from the Sun on the 22nd, 47° west of the Sun. Venus will be easy to spot moving from the constellation Sagittarius into Capricornus shining at magnitude -4.6 on the 15th.|
|Earth - Daylight Savings Time begins at 2 a.m. local time for most of the US on the 9th. The Vernal equinox occurs at 12:57 p.m. EDT on the 20th.|
|Mars - Is stationary on the 1st. Mars rises at 9:30 p.m. on the 1st and about 7:59 p.m. by month's end. Mars viewing is getting better and better as it approaches opposition next month, so get out those binoculars and telescopes and observe Mars in the evenings this month. Mars is in the constellation of Virgo this month shining at magnitude -0.9.|
|Jupiter - Is stationary on the 6th. Jupiter still shines brilliantly in the evening sky this month. Jupiter sets at 3:36 a.m. on the 1st and about 2:38 a.m. by month's end. Look for Jupiter in the evening and early morning skies after midnight. Jupiter is in the constellation of Gemini shining at magnitude -2.3.|
|Saturn - Is stationary on the 2nd. Saturn rises at 11:39 a.m. on the 1st and about 10:33 p.m. by month's end. Look for Saturn rising in the east in late evening. Saturn is in the constellation of Libra shining at magnitude 0.4.|
|Uranus - Sets at 8:16 p.m. on the 1st and about 7:23 p.m. by month's end. Uranus is visible in the early evening sky after sunset. Spot Uranus with binoculars or a small telescope. Uranus is in the constellation of Pisces shining at magnitude 5.9.|
|Neptune - Has returned to the morning sky this month. Neptune rises at 6:23 a.m. on the 1st and about 5:24 a.m. by month's end. Neptune is still lost in the pre-dawn sky until later in the month, though it will still be difficult to spot. Neptune is in the constellation of Aquarius shining at magnitude 8.0.|
|Ceres - Is stationary on the 1st. Ceres rises at 9:33 p.m. on the 1st and about 9:12 p.m. by month's end. Ceres is in the constellation of Virgo shining at magnitude 7.5.|
Rises at 3:25 a.m. on the 1st and about 2:25 a.m. by month's end. Pluto is in the constellation of Sagittarius shining at magnitude 14.2.
As always, good luck at spotting Neptune, Ceres and Pluto, a large telescope and dark skies will be needed.
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For more information about Meteor Showers, visit Gary Kronk's Meteor Showers Online web page.
Elements and Ephemeris for Comet C/2012 S1 (ISON)
For more information about Comets, visit Gary Kronk's Cometography.com webpage.
(From west to east)
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|Cassini - February 24, 2014
Dusty D Ring
Raw images are available at http://saturn.jpl.nasa.gov/photos/raw/index.cfm.
|New Horizons - February 27, 2014
New Horizons Reaches the Final 4 (AU)
"New Horizons sailed past another milepost today when the NASA spacecraft moved to within four astronomical units (AU) of Pluto - which is less than four times the distance between the Earth and the sun, or about 371 million miles (598 million kilometers).
"We're as close to the Pluto system now as Earth ever gets to Jupiter, a first for any spacecraft," says New Horizons Principal Investigator Alan Stern, of the Southwest Research Institute, Boulder, Colo. "And hold on to your hat, it just gets more and more exciting from here."
Since launch on January 19, 2006, New Horizons has covered nearly 2.89 billion miles (4.62 billion kilometers). It makes a temporal connection with one NASA's legendary deep-space explorers this summer when it crosses the orbit of Neptune on Aug. 25 -- exactly 25 years after Voyager 2 made its historic flight past that giant planet. When New Horizons arrives at Pluto on July 14, 2015, it will have traveled farther than any spacecraft ever has to reconnoiter its prime target."
On Video: How Do We Get to Pluto? Practice, Practice, Practice
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.
|Dawn - January 22, 2014
Herschel Telescope Detects Water on Dwarf Planet
Full image and caption
"Scientists using the Herschel space observatory have made the first definitive detection of water vapor on the largest and roundest object in the asteroid belt, Ceres.
Plumes of water vapor are thought to shoot up periodically from Ceres when portions of its icy surface warm slightly. Ceres is classified as a dwarf planet, a solar system body bigger than an asteroid and smaller than a planet.
Herschel is a European Space Agency (ESA) mission with important NASA contributions. "This is the first time water vapor has been unequivocally detected on Ceres or any other object in the asteroid belt and provides proof that Ceres has an icy surface and an atmosphere," said Michael Küppers of ESA in Spain, lead author of a paper in the journal Nature.
The results come at the right time for NASA's Dawn mission, which is on its way to Ceres now after spending more than a year orbiting the large asteroid Vesta. Dawn is scheduled to arrive at Ceres in the spring of 2015, where it will take the closest look ever at its surface."
A gallery of images can be found online.
For more information on the Dawn mission, visit the Dawn home page.
|MESSENGER - February 6, 2014
MESSENGER Surpasses 200,000 Orbital Images of Mercury
"MESSENGER has now returned more than 200,000 images acquired from orbit about Mercury. The 1996 proposal for the mission promised a return of at least 1,000 images says Robert Gold, MESSENGER's Science Payload Manager. "We expected then that we would have some data compression that would probably raise the image total to somewhere near 2,000 images," says Gold, of the Johns Hopkins University Applied Physics Laboratory (APL), but scientists did not imagine then the degree to which MESSENGER would surpass that goal.
"Returning over 200,000 images from orbit about Mercury is an impressive accomplishment for the mission, and one I've been personally counting down for the last few months," says APL's Nancy Chabot, the Instrument Scientist for the Mercury Dual Imaging System (MDIS). "However, I'm really more excited about the many thousands of images that are still in MESSENGER's future, especially those that we plan to acquire at low altitudes and will provide the highest resolution views yet of Mercury's surface."
During MESSENGER's second extended mission, the spacecraft is making a progressively closer approach to Mercury's surface with each successive orbit. In about two months, each closest approach will be at a lower altitude than at any previous point in the mission, enabling the acquisition of unprecedentedly high-spatial-resolution data. For spacecraft altitudes below 350 kilometers, Narrow Angle Camera (NAC) images will be acquired with pixel scales ranging from 20 meters to as little as 2 meters.
To commemorate the milestone, image scientists released this four-image mosaic -- one of the first from the MDIS low-altitude imaging campaign -- that reveals, among other features, hollows that appear to have formed in one layer in the wall of this 15-kilometer-diameter crater."
The MESSENGER app is available for download from iTunes.
For more information on the MESSENGER mission, visit the MESSENGER home page.
|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.
|Past, Present, Future and Proposed JPL Missions - http://www.jpl.nasa.gov/missions
Visit JPL's mission pages for current status.
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Mars website mobile version is here!
| Mars on the Go! NASA Be A Martian Mobile App
If you want the latest news as it happens, try our Be A Martian app.
Download on Mobile Devices
Android | iPhone | Windows Phone
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.
|Mars Science Laboratory - Curiosity - February 19, 2014
Curiosity Adds Reverse Driving for Wheel Protection
"Terrain that NASA's Curiosity Mars rover is now crossing is as smooth as team members had anticipated based on earlier images from orbit. On Tuesday, Feb. 18, the rover covered 329 feet (100.3 meters), the mission's first long trek that used reverse driving and its farthest one-day advance of any kind in more than three months.
The reverse drive validated feasibility of a technique developed with testing on Earth to lessen damage to Curiosity's wheels when driving over terrain studded with sharp rocks. However, Tuesday's drive took the rover over more benign ground.
"We wanted to have backwards driving in our validated toolkit because there will be parts of our route that will be more challenging," said Curiosity Project Manager Jim Erickson of NASA's Jet Propulsion Laboratory, Pasadena, Calif.
The rover team used images taken from orbit to reassess possible routes, after detecting in late 2013 that holes in the vehicle's aluminum wheels were accumulating faster than anticipated. Getting to the chosen route, which appeared to be less hazardous for the wheels, required crossing a 3-foot-tall (1-meter-tall) dune. Curiosity crossed the dune on Feb. 9.
Erickson said, "After we got over the dune, we began driving in terrain that looks like what we expected based on the orbital data. There are fewer sharp rocks, many of them are loose, and in most places there's a little bit of sand cushioning the vehicle."
The mission's destinations remain the same: a science waypoint first and then the long-term goal of investigating the lower slopes of Mount Sharp, where water-related minerals have been detected from orbit."
For information about NASA's partnership with Foursquare, visit:http://www.nasa.gov/connect/foursquare.html.
Mars Rover Landing - Free for the Xbox (requires Kinect)
Visit the Mars Science Laboratory page.
|Mars Exploration Rover Mission (Spirit and Opportunity) - January 23, 2013
SPIRIT UPDATE: Spirit Remains Silent at Troy - sols 2621-2627, May 18-24, 2011:
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: Busy Week of Imaging and Robotic Arm Studies - sols 3568-3575, Feb. 05, 2014-Feb. 12, 2014 :
"Opportunity is climbing 'Murray Ridge' up on Solander Point, part of the rim of Endeavour Crater.
The rover continues to explore the region called 'Cook Haven.' The rover has turned its attention to other rocks within this area. On Sol 3568 (Feb. 5, 2014), Opportunity lifted her robotic arm so 13-filter Panoramic Camera (Pancam) images of the surface target, called 'Green Island' could be collected, along with some Navigation (Navcam) images. On the next sol, the rover used the Rock Abrasion Tool (RAT) to brush a spot on Green Island and followed that with a Microscopic Imager (MI) mosaic and a placement of the Alpha Particle X-ray Spectrometer (APXS).
On Sol 3571 (Feb. 8, 2014), the rover collected a 13-filter Pancam image of the brushed spot on Green Island before bumping about 9.8 feet (3 meters) to a new rock target, called 'Stuart Island.' Opportunity began the in-situ (contact) investigation of Stuart Island on Sol 3573 (Feb. 10, 2014), with a MI mosaic and APXS placement for an overnight integration. The rover repeated this again on the next sol with more MI mosaics, but with an offset placement of the APXS. Continuing the campaign on Sol 3575 (Feb. 12, 2014), Opportunity collected more MI mosaics and performed a third offset of the APXS.
As of Sol 3575 (Feb. 12, 2014), the solar array energy production was 387 watt-hours with an atmospheric opacity (Tau) of 0.548 and a solar array dust factor of 0.610.
Total odometry is 24.07 miles (38.74 kilometers)."
Visit the Mars Exploration Rover page.
|Mars Reconnaissance Orbiter Mission - February 19, 2014
Mars Orbiter Images Rover and Tracks in Gale Crater
"A new image from a telescopic camera orbiting Mars shows NASA's Mars Exploration Rover Opportunity at work on "Murray Ridge," without any new impact craters nearby.
The Feb. 14 view from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is available online at http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA17941. Rover tracks from Opportunity, as well as the rover itself, are visible.
A rock, dubbed "Pinnacle Island," appeared in January 2014 next to Opportunity where it had been absent a few days earlier. After that, researchers using HiRISE planned this observation to check the remote possibility that a fresh impact by an object from space might have excavated a crater near Opportunity and thrown this rock to its new location. No fresh impact site is seen in the image. Meanwhile, observations by the rover solved the Pinnacle Island mystery by finding where the rock had been struck, broken and moved by a rover wheel.
Murray Ridge is part of the western rim of Endeavour Crater, an impact scar that is billions of years old and about 14 miles (22 kilometers) in diameter."
MARS RECONNAISSANCE ORBITER HIRISE IMAGES
More information about the MRO mission is available online.
|Mars Odyssey Orbiter - February 12, 2014
NASA Moves Longest-Serving Mars Spacecraft for New Observations
"NASA's Mars Odyssey spacecraft has tweaked its orbit to help scientists make the first systematic observations of how morning fogs, clouds and surface frost develop in different seasons on the Red Planet.
The maneuver took place Tuesday, Feb. 11. Odyssey team engineers at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and Lockheed Martin Space Systems of Denver, designed the gentle move to accelerate Odyssey's drift toward a morning-daylight orbit. The desired change will occur gradually until the intended orbit geometry is reached in November 2015 and another maneuver halts the drift.
The change will enable observation of changing ground temperatures after sunrise and after sunset in thousands of places on Mars. Those observations could yield insight about the composition of the ground and about temperature-driven processes, such as warm-season flows observed on some slopes, and geysers fed by spring thawing of carbon-dioxide ice near Mars' poles.
"We're teaching an old spacecraft new tricks," said Odyssey Project Scientist Jeffrey Plaut of JPL. "Odyssey will be in position to see Mars in a different light than ever before."
Neither Odyssey, nor any other NASA Mars orbiter since the 1970s, has flown an orbital pattern with a view of the ground in morning daylight. Earlier NASA orbiters and the European Space Agency's Mars Express orbiter have provided some tantalizing views of morning mists on Mars, but have concentrated on afternoon observation times when views of the surface are less hazy.
Odyssey was launched in 2001 and began its science mission 12 years ago this month. It is the longest-working spacecraft ever sent to Mars."
"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.
|Mars Missions Status|
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More Acknowledgements and References
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