Dunes in the spring
A piece of Mars: Dunes near the north and south poles get cold in the winter, just like they do on Earth. Except on Mars instead of H2O ice, it’s a mix of CO2 and H2O ice (mostly CO2). In the spring the white ice slowly disappears, revealing the dark dunes underneath. (HiRISE PSP_002033_1325, NASA/JPL/University of Arizona)
- aeolian | dunes | ice
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Progress on the GPI exoplanet imager integration
The Gemini Planet Imager (GPI) is a next generation adaptive optics instrument being built for the Gemini Observatory. This is an ambitious project with the goal of directly imaging extrasolar planets orbiting nearby stars. The instrument is currently being integrated at the University of California at Santa Cruz. After more than a year of testing in a fixed orientation in a clean room, on March 7, 2013, the 2,030 kg instrument was set up on a crane and flexure rig. In collaboration with the UCSC team, we prepared this time lapse video showing GPI being set up in its new position.
- exoplanets | Gemini Planet Imager | GPI | Integration | UCSC
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Progress on the GPI exoplanet imager integration
The Gemini Planet Imager (GPI) is a next generation adaptive optics instrument being built for the Gemini Observatory. This is an ambitious project with the goal of directly imaging extrasolar planets orbiting nearby stars. The instrument is currently being integrated at the University of California at Santa Cruz. After more than a year of testing in a fixed orientation in a clean room, on March 7, 2013, the 2,030 kg instrument was set up on a crane and flexure rig. In collaboration with the UCSC team, we prepared this time lapse video showing GPI being set up in its new position.
- Gemini | Gemini Planet Imager | GPI | imaging exoplanets | UCSC
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Nili Patera
A piece of Mars: Nili Patera on Mars is an ancient volcano. Some of the old volcanic material has been blown into rather striking sand dunes. It is the first place where dunes were conclusively identified as actively moving. Here’s a closeup of one of them — the steep slip face on the downwind side indicates these dunes are moving to the lower left. This dune migrates about a meter every year. (HiRISE ESP_030210_1890, NASA/JPL/University of Arizona)
- active | aeolian | dunes
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A piece of Mars: Here are some old dunes that look a little like vertebrae of fossils (if you think they look like dragon spines poking out of the ground then you’re playing too many video games). The white areas are stabilized and possibly lithified. The blue areas are where the dunes are being actively eroding, exposing old bedding (faint parallel stripes) within the dunes. (HiRISE ESP_030583_1610, NASA/JPL/University of Arizona)
- aeolian | crossbedding | erosion | stabilized
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Almost a dune
A piece of Mars: Not all piles of windblown sand are able to form proper dunes, with a fully developed avalanche on the downwind side. Here, bluish sand tries to make its way through hilly terrain, which both traps the sand and makes it difficult for slip faces (avalanches) to form. Smaller, now stabilized dunes in the upper right were also trapped by the hills. (HiRISE ESP_030570_1440, NASA/JPL/University of Arizona)
- aeolian | stabilized
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Featuring the Women Of Science #WomenOfScience
Today I would like to share with you an idea for the International Women’s day on March 8 2013. If you work in an institution, university, or non-profit related to science, have you taken note of the number of women around you? In astronomy and planetary science, it is not too bad even if it is not perfect, but some “hard” science groups, like physics or computer science, clearly have a low proportion of women in their ranks. I will not elaborate on the reasons for such lack of representation; instead, I propose to focus on the bright side.
- Diversity | Science | SETI Institute | Women Of Science
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Windswept landscape
A piece of Mars: As the wind blows sand over terrain, the grains deepen grooves in weak materials, enhancing the topography in the direction of the strongest wind. Here, over eons, sand marching from right to left has formed dunes (oriented perpendicular to the wind) and elongated grooves downwind of low hills. (HiRISE ESP_030582_1850, NASA/JPL/University of Arizona)
- aeolian | dunes | erosion
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Those feathery bright dunes on Mars
A piece of Mars: Some of the dunes on Mars are just plain weird. Here are some feather-shaped ones. I’m not sure anybody knows why they form these fractal shapes just yet. I don’t know of anything on Earth that looks like these. (HiRISE ESP_028024_1830 NASA/JPL/University of Arizona)
- aeolian | dunes | erosion | stabilized
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Drifting sand
A piece of Mars: Dark sand has been blown into the scene from the upper right. It has piled up against older, brighter dunes that may now be inactive. The sand drifts on and on, piling up where the wind weakens and carving out rock where the wind is strong. And that is geology on Mars today. (HiRISE ESP_028024_1830 NASA/JPL/University of Arizona)
- aeolian | dunes | stabilized
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