Image Credit: NASA/ESA/Samantha Cristoforetti via NASA http://ift.tt/1CLJOYl
Tag Archives: NASA
Hubble’s Little Sombrero
This is NGC 7814, also known as the “Little Sombrero.” Its larger namesake, the Sombrero Galaxy, is another stunning example of an edge-on galaxy — in fact, the “Little Sombrero” is about the same size as its bright namesake at about 60,000 light-years across, but as it lies farther away, and so appears smaller in the sky.
NGC 7814 has a bright central bulge and a bright halo of glowing gas extending outwards into space. The dusty spiral arms appear as dark streaks. They consist of dusty material that absorbs and blocks light from the galactic center behind it. The field of view of this NASA/ESA Hubble Space Telescope image would be very impressive even without NGC 7814 in front; nearly all the objects seen in this image are galaxies as well.
European Space Agency
Credit: ESA/Hubble & NASA
Acknowledgement: Josh Barrington via NASA http://ift.tt/16prBlg
Forty-Four Years Ago Today: Apollo 14 Touches Down on the Moon
Image Credit: NASA via NASA http://ift.tt/1zjYwTG
Curiosity Rover at ‘Pahrump Hills’
The location of the rover, with its shadow extending toward the upper right, is indicated with an inscribed rectangle. Figure A is an unannotated version of the image. North is toward the top. The view covers an area about 360 yards (330 meters) across.
HiRISE made the observation on Dec. 13, 2014. At that time, Curiosity was near a feature called “Whale Rock.” A map showing the rover’s path for the weeks leading up to that date is at http://ift.tt/1DeDac2 . The inset map at http://ift.tt/16owOdk labels the location of Whale Rock and other features in the Pahrump Hills area.
The bright features in the landscape are sedimentary rock and the dark areas are sand. The HiRISE team plans to periodically image Curiosity, as well as NASA’s other active Mars rover, Opportunity, as the vehicles continue to explore Mars.
This image is an excerpt from HiRISE observation ESP_039280_1755. Other image products from this observation are available at http://ift.tt/16owPha .
The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colorado. NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project and Mars Science Laboratory Project for NASA’s Science Mission Directorate, Washington.
Image Credit: NASA/JPL-Caltech/Univ. of Arizona via NASA http://ift.tt/1BUWhDB
‘State of NASA’ Address at Kennedy Space Center
Photo credit: NASA/Amber Watson via NASA http://ift.tt/1zDuXgo
Cloud Streets in the Bering Sea
The frozen tundra of Russia lies in the northwest of the image, and snow-covered Alaska lies in the northeast. Sea ice extends from the land well into the Bering Sea. Over the dark water bright white clouds line in up close, parallel rows. These formations are known as “cloud streets”.
Air blowing over the cold, snowy land and then over ice becomes both cold and dry. When the air then moves over relatively warmer and much moister water and lead to the development of parallel cylinders of spinning air. On the upper edge of these cylinders of air, where the air is rising, small clouds form. Where air is descending, the skies are clear. This clear/cloudy pattern, formed in parallel rows, gives the impression of streets.
The clouds begin over the sea ice, but they primarily hang over open ocean. The streets are neat and in tight rows closest to land, while further over the Bering Sea the pattern widens and begins to become more random. The rows of clouds are also not perfectly straight, but tend to curve. The strength and direction of the wind helps create these features: where the wind is strongest, nearest to shore, the clouds line up most neatly. The clouds align with the wind direction, so the direction of the streets gives strong clues to prevailing wind direction.
Image Credit: NASA/Jeff Schmaltz, MODIS Land Rapid Response Team, NASA GSFC via NASA http://ift.tt/1z6p62x
Super View of Glendale and Phoenix
Image Credit: NASA via NASA http://ift.tt/1wSk6ZU
SMAP Takes to the Skies
Hubble’s View of the Polar Ring of Arp 230
Arp 230 is a galaxy of an uncommon or peculiar shape, and is therefore part of the Atlas of Peculiar Galaxies produced by Halton Arp. Its irregular shape is thought to be the result of a violent collision with another galaxy sometime in the past. The collision could also be held responsible for the formation of the galaxy’s polar ring.
The outer ring surrounding the galaxy consists of gas and stars and rotates over the poles of the galaxy. It is thought that the orbit of the smaller of the two galaxies that created Arp 230 was perpendicular to the disk of the second, larger galaxy when they collided. In the process of merging the smaller galaxy would have been ripped apart and may have formed the polar ring structure astronomers can observe today.
Arp 230 is quite small for a lenticular galaxy, so the two original galaxies forming it must both have been smaller than the Milky Way. A lenticular galaxy is a galaxy with a prominent central bulge and a disk, but no clear spiral arms. They are classified as intermediate between an elliptical galaxy and a spiral galaxy.
European Space Agency
Image Credit: ESA/Hubble & NASA, Acknowledgement: Flickr user Det58 via NASA http://ift.tt/1yLHxoB
Delta II Rocket With Soil Moisture Active Passive (SMAP) Mission Onboard
Image Credit: NASA/Bill Ingalls via NASA http://ift.tt/1Kbxxvx