Showing posts with label THEMIS. Show all posts
Showing posts with label THEMIS. Show all posts

Tuesday, May 4, 2010

Mars Odyssey THEMIS images - April 26-30, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Auqakuh Vallis (Released 26 April 2010)
    This VIS image shows a small portion of Auqakuh Vallis.
  • Daedalia Planum (Released 27 April 2010)
    Some of the youngest volcanic flows on Mars are from Arsia Mons.
  • Ascraeus Mons (Released 28 April 2010)
    This VIS image shows part of the northeastern flank of Ascraeus Mons, one of the large Tharsis volcanoes.
  • Juventae Chasma (Released 29 April 2010)
    Baetis Chasma is a chasmata near Valles Marineris.
  • Galaxias Fossae (Released 30 April 2010)
    The fracture system in this VIS image is part of Galaxias Fossae, a series of fractures on the northern part of the Elysium Mons volcanic complex.

Wednesday, April 28, 2010

Asteroid Ice May Be Living Fossil With Clues To Oceans' Origins


The first-ever discovery of ice and organic molecules on an asteroid may hold clues to the origins of Earth's oceans and life 4 billion years ago.

University of Central Florida researchers detected a thin layer of water ice and organic molecules on the surface of 24 Themis, the largest in a family of asteroids orbiting between Mars and Jupiter.

Their unexpected findings will be published in Nature, which will featuretwo complementary articles by the UCF-led team and by another team of planetary scientists.

"What we've found suggests that an asteroid like this one may have hit Earth and brought our planet its water," said UCF Physics Professor HumbertoCampins, the study's lead author.

Some theories suggest asteroids brought water to Earth after the planet formed dry. Scientists say the salts and water that have been found in some meteorites support this view.

Using NASA's Infrared Telescope Facility in Hawaii, Campins and his team of researchers measured the intensity of the reflected sunlight as 24 Themis rotated. Differences in intensity at different wavelengths helped researchers determine the makeup of the asteroid's surface.

Researchers were surprised to find ice and carbon-based compounds evenly distributed on 24 Themis. More specifically, the discovery of ice is unexpected because surface ice should be short lived on asteroids, which are expected to be too warm for ice to survive for long.

The distance between this asteroid and the sun is about three times greater than between Earth and the sun.

Researchers will continue testing various hypotheses to explain the presence of ice. Perhaps most promising is the possibility that 24 Themis might have preserved the ice in its subsoil, just below the surface, as a kind of "living fossil" or remnant of an early solar system that was generally considered to have disappeared long ago.


Scientists Finds Evidence Of Water Ice On Asteroid's Surface


This image shows the Themis Main Belt which sits between Mars and Jupiter. Asteroid 24 Themis, one of the largest Main Belt asteroids, was examined by University of Tennessee scientist, Josh Emery, who found water ice and organic material on the asteroid's surface. His findings were published in the April 2010 issue of Nature. Credit: Josh Emery/University of Tennessee, Knoxville

Asteroids may not be the dark, dry, lifeless chunks of rock scientists have long thought.

Josh Emery, research assistant professor with the earth and planetary sciences department at the University of Tennessee, Knoxville, has found evidence of water ice and organic material on the asteroid 24 Themis. This evidence supports the idea that asteroids could be responsible for bringing water and organic material to Earth.

The findings are detailed in the journal "Nature."

Using NASA's Infrared Telescope Facility on Hawaii's Mauna Kea, Emery and Andrew Rivkin of Johns Hopkins University in Laurel, Md., examined the surface of 24 Themis, a 200-kilometer wide asteroid that sits halfway between Mars and Jupiter.

By measuring the spectrum of infrared sunlight reflected by the object, the researchers found the spectrum consistent with frozen water and determined that 24 Themis is coated with a thin film of ice. They also detected organic material.

"The organics we detected appear to be complex, long-chained molecules. Raining down on a barren Earth in meteorites, these could have given a big kick-start to the development of life," Emery said.

Emery noted that finding ice on the surface of 24 Themis was a surprise because the surface is too warm for ice to stick around for a long time.

"This implies that ice is quite abundant in the interior of 24 Themis and perhaps many other asteroids. This ice on asteroids may be the answer to the puzzle of where Earth's water came from," he said.

Still, how the water ice got there is unclear.

24 Themis' proximity to the sun causes ice to vaporize. However, the researchers' findings suggest the asteroid's lifetime of ice ranges from thousands to millions of years depending on the latitude.

Therefore, the ice is regularly being replenished. The scientists theorize this is done by a process of "outgassing" in which ice buried within the asteroid escapes slowly as vapor migrates through cracks to the surface or as vapor escapes quickly and sporadically when 24 Themis is hit by space debris.

Since Themis is part of an asteroid "family" that was formed from a large impact and the subsequent fragmentation of a larger body long ago, this scenario means the parent body also had ice and has deep implications for how our solar system formed.

The discovery of abundant ice on 24 Themis demonstrates that water is much more common in the Main Belt of asteroids than previously thought.

"Asteroids have generally been viewed as being very dry. It now appears that when the asteroids and planets were first forming in the very early Solar System, ice extended far into the Main Belt region," Emery said.

"Extending this refined view to planetary systems around other stars, the building blocks of life - water and organics - may be more common near each star's habitable zone. The coming years will be truly exciting as astronomers search to discover whether these building blocks of life have worked their magic there as well."

The scientists' discovery also further blurs the line between comets and asteroids. Asteroids have long been considered to be rocky and comets icy. Furthermore, it was once believed that comets could have brought water to Earth. This theory was nixed when it was discovered comets' water has different isotopic signatures than water on Earth.

Now, due to Emery and Rivkin's findings, many wonder if asteroids could be responsible for seeding Earth with the ingredients for life.

Tuesday, April 20, 2010

Mars Odyssey THEMIS images - April 12-16, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Candor Chasma (Released 12 April 2010)
    This VIS image of Candor Chasma contains eroded deposits of material and a large landslide deposit.
  • Hecates Tholus (Released 13 April 2010)
    This VIS image shows the southeastern flank of Hecates Tholus, the northernmost volcano of the Elysium Volcanic complex.
  • Terra Sabaea (Released 14 April 2010)
    The northern part of Terra Sabaea is heavily fractured and channeled, breaking up into a chaotic terrain as the elevation drops down to the northern plains.
  • Arabia Terra (Released 15 April 2010)
    Dark slope streaks mark this crater rim.
  • Coprates Chasma (Released 16 April 2010)
    This VIS image shows a portion of the floor of Coprates Chasma.

Saturday, April 10, 2010

Mars Odyssey THEMIS images - April 5-9, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Arsia Mons Flows (Released 5 April 2010)
    The lava flows in this VIS image are part of the extensive flow field of Arsia Mons.
  • Arkhanglesky Crater Dunes (Released 6 April 2010)
    This VIS image shows part of the dune field located on the floor of Arkhangelsky Crater.
  • Wind Effects (Released 7 April 2010)
    This VIS image shows some of the effects that wind action has on the surface of Mars.
  • Sabis Vallis (Released 8 April 2010)
    A section of Sabis Vallis is shown in today's VIS image.
  • Eastern Coprates Chasma (Released 9 April 2010)
    This VIS image of the eastern end of Coprates Chasma contains a landslide deposit and sand dunes.

Thursday, April 8, 2010

HiRISE images for April 7, 2010


The following new captioned and spotlight images taken by the High Resolution Imaging Science Experiment (HiRISE) on the Mars Reconnaissance Orbiter spacecraft are now available:
  • Faulted Layered Bedrock in Noctus Labyrinthus
    A portion of this observation shows layered bedrock that has been faulted and tilted.
  • Fading Young Impact Crater
    This image shows a new impact crater that formed on Mars between May 2002 and February 2004. It was discovered in data from the Mars Odyssey Mission THEMIS instrument and later confirmed to be an impact crater by the Context Camera on Mars Reconnaissance Orbiter.
  • Monitor Spirit Landing Site for Aeolian Changes
    This observation covers the Columbia Hills and the surrounding plains of Gusev Crater, which the Mars Exploration Rover Spirit has been exploring since January 2004. Repeat images of this site have been acquired to study aeolian (wind-related) changes on the surface.
  • Polygonal Patterned Ground
    From a distance, the floor of this crater looks like a giant honeycomb or spider web. The intersecting shapes, or polygons, commonly occur in the northern lowlands of Mars.
  • Avalanche Clouds
    This HiRISE image shows at least three isolated clouds of particles near a steep cliff in the northern polar region of Mars.

Friday, April 2, 2010

Mars Odyssey THEMIS images - March 29-April 2, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Ceranus Tholus (Released 29 March 2010)
    This VIS image shows the western edge of the summit caldera of Ceranus Tholus, one of the smaller volcanic constructs of the Tharsis region.
  • Coprates Catena (Released 30 March 2010)
    This VIS image shows a small portion of the floor of Coprates Catena.
  • Tithonium Chasma (Released 31 March 2010)
    Today's VIS image is of part of Tithonium Chasma, part of the western side of Valles Marineris.
  • Aurorae Chaos (Released 1 April 2010)
    The landslide deposit in this VIS image is located in Aurorae Chaos.
  • Bahram Vallis (Released 2 April 2010)
    This VIS image shows a section of Bahram Vallis.

Monday, March 22, 2010

Mars Odyssey THEMIS images - Feb 22-24 and Mar 15-19 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Gale Crater (Released 22 February 2010)
    This VIS image shows a portion of the rim and floor of Gale Crater.
  • Dunes (Released 23 February 2010)
    This dunes in this VIS image are located on the floor of an unnamed crater in Tyrrhena Terra.
  • Pasteur Crater (Released 24 February 2010)
    The small, dark features in this VIS image are sand dunes.
  • Sand Dunes (Released 15 March 2010)
    A sand dune field is located on the floor of this unnamed crater in Terra Cimmeria.
  • Candor Chasma (Released 17 March 2010)
    This large landslide is located in Candor Chasma.
  • McLaughlin Crater Dunes (Released 18 March 2010)
    These sand dunes are located on the floor of McLaughlin Crater.
  • Candor Chasma (Released 19 March 2010)
    The ridge features at the top of this VIS image are called spurs.

Sunday, March 21, 2010

Mars Odyssey THEMIS images - Feb 22-24 and Mar 15-19 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Gale Crater (Released 22 February 2010)
    This VIS image shows a portion of the rim and floor of Gale Crater.
  • Dunes (Released 23 February 2010)
    This dunes in this VIS image are located on the floor of an unnamed crater in Tyrrhena Terra.
  • Pasteur Crater (Released 24 February 2010)
    The small, dark features in this VIS image are sand dunes.
  • Sand Dunes (Released 15 March 2010)
    A sand dune field is located on the floor of this unnamed crater in Terra Cimmeria.
  • Candor Chasma (Released 17 March 2010)
    This large landslide is located in Candor Chasma.
  • McLaughlin Crater Dunes (Released 18 March 2010)
    These sand dunes are located on the floor of McLaughlin Crater.
  • Candor Chasma (Released 19 March 2010)
    The ridge features at the top of this VIS image are called spurs.

Wednesday, February 24, 2010

Mars Odyssey THEMIS images - February 8-19, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Tithonium Chasma (Released 8 February 2010)
    Two landslide deposits are visible in this image of Tithonium Chasma.
  • Coprates Chasma (Released 9 February 2010)
    This VIS image of Coprates Chasma shows several landslide deposits.
  • Coprates Catena (Released 10 February 2010)
    The interconnected collapse pits at the top of this VIS image are part of Coprates Catena.
  • Dark Slope Streaks (Released 11 February 2010)
    Numerous dark slope streaks are visible in this small unnamed crater in Zephyria Planum.
  • Dunes (Released 12 February 2010)
    The dunes in this VIS image are located on the floor of an unnamed crater in Tyrrhena Terra.

Friday, February 12, 2010

Mars Odyssey THEMIS images - February 1-5, 2010


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Proctor Crater Dunes (Released 1 February 2010)
    This VIS image of the floor of Proctor Crater shows part of the sand sheet and dune forms that are located there.
  • Arkhangelsky Crater (Released 2 February 2010)
    This VIS image shows part of the floor of Arkhangelsky Crater.
  • Lycus Sulci (Released 3 February 2010)
    Dark slope streaks are found throughout Lycus Sulci.
  • Patapsco Vallis (Released 4 February 2010)
    This VIS image shows a portion of Patapsco Vallis, a channel located on the eastern margin of Elysium Mons.
  • Coprates Chasma (Released 5 February 2010)
    The floor of Coprates Chasma contains many different geologic landforms.

Sunday, December 6, 2009

Mars Odyssey THEMIS images - November 23-27, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Dunes (Released 23 November 2009)
    This VIS image shows a portion of a dune field on the floor of an unnamed crater in Noachis Terra.
  • Lycus Sulci (Released 24 November 2009)
    Lycus Sulci is a very complex region surrounding the northern flank of Olympus Mons.
  • Windstreaks (Released 25 November 2009)
    The windstreaks in this VIS image are located in Syrtis Major Planum.
  • Brashear Crater Dunes (Released 26 November 2009)
    This VIS image shows the dune field on the floor of Brashear Crater.
  • Arsia Mons Flows (Released 27 November 2009)
    This VIS image shows lava flows of Arsia Mons.

Monday, July 13, 2009

Mars Odyssey THEMIS images - July 6-10, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Nirgal Vallis (Released 6 July 2009)
    This VIS image shows a portion of Nirgal Vallis and a scalloped tributary channel.
  • Holden Crater (Released 7 July 2009)
    This daytime infrared image shows the dissection of the rim of Holden Crater by numerous channels.
  • Polar Layers (Released 8 July 2009)
    The numerous layers of the south polar cap are shown in cross-section in this VIS image.
  • Dust Devil Tracks (Released 9 July 2009)
    The plains of Planum Chronium shown in this VIS images are covered by hundreds of dust devil tracks.
  • Rabe Crater (Released 10 July 2009)
    This daytime infrared image of Rabe Crater illustrates the warming effect of the sun on sand.

Monday, July 6, 2009

Mars Odyssey THEMIS images - June 29-July 3, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Lycus Sulci (Released 29 June 2009)
    Dark slope streaks are common in Lycus Sulci.
  • Lipik Channels (Released 30 June 2009)
    This daytime infrared image clearly shows the multitude of channels dissecting the rim of Lipik Crater.
  • Polar Dune (Released 1 July 2009)
    A large sand sheet with surface dune forms is located on the floor of this crater near the south pole.
  • Dunes (Released 2 July 2009)
    Small, dark dunes are found on the floor of this crater near Meridiani Planum.
  • Dust Devil Tracks (Released 3 July 2009)
    Faint dust devil tracks can be seen in the VIS image.

Sunday, June 28, 2009

Mars Odyssey THEMIS images - June 22-26, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Unusual Textures (Released 22 June 2009)
    Odd rimmed depressions are located on the floor of this unnamed crater in Noachis Terra.
  • Coprates Chasma (Released 23 June 2009)
    This VIS image crosses Coprates Chasma, showing both floor and wall features of the canyon.
  • Sirenum Fossae (Released 24 June 2009)
    This VIS image shows a portion of the eastern end of Sirenum Fossae.
  • Sirenum Fossae (Released 25 June 2009)
    This VIS image of the western portion of Sirenum Fossae shows mesa formation.
  • Olympus Mons (Released 26 June 2009)
    This VIS image shows flow features on the northern flank of Olympus Mons.

Sunday, June 21, 2009

Mars Odyssey THEMIS images - June 15-19, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Proctor Crater Dunes (Released 15 June 2009)
    This infrared (IR) image of Proctor Crater shows the dune field on the floor of the crater.
  • Landslide (Released 16 June 2009)
    This VIS image shows a landslide in Capri Chasma.
  • Southern Crater Dunes (Released 17 June 2009)
    Many craters around the south polar cap contain dune fields on their floors.
  • Channel (Released 18 June 2009)
    This in an IR image of an unnamed channel in northwestern Terra Cimmeria.
  • Channel (Released 19 June 2009)
    This VIS image shows a channel with extensive scalloping of its margins.

Saturday, June 13, 2009

Mars Odyssey THEMIS images - June 9-12, 2009


The following new images taken by the Thermal Emission Imaging System (THEMIS) on the Mars Odyssey spacecraft are now available:
  • Polar Ridges (Released 9 June 2009)
    Intersecting linear ridges are found in several locations around the south polar cap.
  • South Polar Textures (Released 10 June 2009)
    As spring turns to summer, the frost cover has been removed from the south polar cap. The surface textures seen in this VIS image are created by action of the sun on the icy cap.
  • Crater Rim Channels (Released 11 June 2009)
    Channels dissect the northern rim of this unnamed crater in Terra Cimmeria.
  • Terby Crater (Released 12 June 2009)
    This VIS image shows some of the eroded, layered crater fill material within Terby Crater.