My God, it’s full
of stars.
This target comes from the public via HiWish: “Similar HiRISE images of mounds around Chryse Planitia have revealed stunning and complex stratigraphy, indicative of widespread, regional-scale processes.”
https://uahirise.org/hipod/ESP_076553_2040
#Mars
This target comes from the public via HiWish: “Similar HiRISE images of mounds around Chryse Planitia have revealed stunning and complex stratigraphy, indicative of widespread, regional-scale processes.”
https://uahirise.org/hipod/ESP_076553_2040
#Mars
The objective of this observation is to examine what appears to be ejecta moving into a small crater. More resolution is needed to tell exactly what is going on here.
https://uahirise.org/hipod/ESP_076514_2070
#Mars #science #NASA
The objective of this observation is to examine what appears to be ejecta moving into a small crater. More resolution is needed to tell exactly what is going on here.
https://uahirise.org/hipod/ESP_076514_2070
#Mars #science #NASA
This image provides a look at layered deposits that with a stereo pair with maximal vertical resolution, can give us some insight into bed thickness measurements.
https://uahirise.org/hipod/ESP_076447_1900
NASA/JPL-Caltech/University of Arizona
#Mars
This image provides a look at layered deposits that with a stereo pair with maximal vertical resolution, can give us some insight into bed thickness measurements.
https://uahirise.org/hipod/ESP_076447_1900
NASA/JPL-Caltech/University of Arizona
#Mars
The CaSSIS instrument on the ExoMars Trace Gas Orbiter identified here extremely red crater rim materials. This appears very bright and distinct in THEMIS (Mars Odyssey) nighttime data as well.
https://uahirise.org/hipod/ESP_076523_1530
#Mars #science #NASA
The CaSSIS instrument on the ExoMars Trace Gas Orbiter identified here extremely red crater rim materials. This appears very bright and distinct in THEMIS (Mars Odyssey) nighttime data as well.
https://uahirise.org/hipod/ESP_076523_1530
#Mars #science #NASA
The objective of this observation is to examine a group of streamlined features. Most of our image footprint is full of these features.
https://uahirise.org/hipod/ESP_076521_2100
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
The objective of this observation is to examine a group of streamlined features. Most of our image footprint is full of these features.
https://uahirise.org/hipod/ESP_076521_2100
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
The apron could be (or could have been) ice-rich, so one possibility is that the fissures are related to ice loss. Scientists think that extensive glaciers covered this region several hundred million years ago.
https://uahirise.org/hipod/ESP_039384_2100
#Mars
The apron could be (or could have been) ice-rich, so one possibility is that the fissures are related to ice loss. Scientists think that extensive glaciers covered this region several hundred million years ago.
https://uahirise.org/hipod/ESP_039384_2100
#Mars
www.forbes.com/sites/caroli...
www.forbes.com/sites/caroli...
These always make me smile
These always make me smile
This observation is based on coverage over existing high-resolution CRISM data that shows a sliver of residual carbon dioxide ice and its margins.
https://uahirise.org/hipod/ESP_076461_0940
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
This observation is based on coverage over existing high-resolution CRISM data that shows a sliver of residual carbon dioxide ice and its margins.
https://uahirise.org/hipod/ESP_076461_0940
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
Also visible in Context Camera image data, the objective of this observation is to examine layers near an impact crater. The shape of this particular formation is striking in its mesa-like appearance.
https://uahirise.org/hipod/ESP_076497_2070
#Mars
Also visible in Context Camera image data, the objective of this observation is to examine layers near an impact crater. The shape of this particular formation is striking in its mesa-like appearance.
https://uahirise.org/hipod/ESP_076497_2070
#Mars
This region hosts remarkably complex dunes like this field in the Hellespontus Montes mountain range. Dunes here migrate both east and west, converging at a central area.
More: https://uahirise.org/hipod/ESP_016339_1380
#Mars #science #NASA
This region hosts remarkably complex dunes like this field in the Hellespontus Montes mountain range. Dunes here migrate both east and west, converging at a central area.
More: https://uahirise.org/hipod/ESP_016339_1380
#Mars #science #NASA
The objective of this observation is to take a cloesr look at a ridge. In some spots, the surfaces on either side of this ridge seem different.
https://uahirise.org/hipod/ESP_076446_2270
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
The objective of this observation is to take a cloesr look at a ridge. In some spots, the surfaces on either side of this ridge seem different.
https://uahirise.org/hipod/ESP_076446_2270
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
The objective of this observation is to examine a channel. There are many channels in this region. The channel makes a sharp turn in our image field.
https://uahirise.org/hipod/ESP_076488_1440
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
The objective of this observation is to examine a channel. There are many channels in this region. The channel makes a sharp turn in our image field.
https://uahirise.org/hipod/ESP_076488_1440
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
This image of a dune field in the polar region of Mars allows us to study long-term weathering patterns.
Full cutout on Flickr: https://flic.kr/p/2rEUcyk
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
This image of a dune field in the polar region of Mars allows us to study long-term weathering patterns.
Full cutout on Flickr: https://flic.kr/p/2rEUcyk
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
The objective of this observation is to examine channels. Some are rather deep, but others that are eroded are small branches.
https://uahirise.org/hipod/ESP_076485_1525
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
The objective of this observation is to examine channels. Some are rather deep, but others that are eroded are small branches.
https://uahirise.org/hipod/ESP_076485_1525
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
Our science objective here is straightfoward: to investigate this interesting fissure geometry and the sourcing channels. This flat, volcanic plain is located directly east of Pavonis Mons.
https://uahirise.org/hipod/ESP_076477_1820
NASA/JPL-Caltech/University of Arizona
Our science objective here is straightfoward: to investigate this interesting fissure geometry and the sourcing channels. This flat, volcanic plain is located directly east of Pavonis Mons.
https://uahirise.org/hipod/ESP_076477_1820
NASA/JPL-Caltech/University of Arizona
In this image we can see many dark streaks extending down the slope, but no sign yet of larger avalanches that were common in past years.
https://uahirise.org/hipod/ESP_068674_2640
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
In this image we can see many dark streaks extending down the slope, but no sign yet of larger avalanches that were common in past years.
https://uahirise.org/hipod/ESP_068674_2640
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
This image shows a surface shaped by ice. Funnel-shaped craters scattered throughout the image are interpreted as impacts that once had the classic bowl shape, but have now expanded via sublimation.
https://uahirise.org/hipod/ESP_069002_2305
#Mars
This image shows a surface shaped by ice. Funnel-shaped craters scattered throughout the image are interpreted as impacts that once had the classic bowl shape, but have now expanded via sublimation.
https://uahirise.org/hipod/ESP_069002_2305
#Mars
This feature was first viewed by the CaSSIS instrument, and is similar to the ones in Nili Fossae. An inverted channel?
https://www.uahirise.org/anaglyph/ESP_089248_2125_ESP_078541_2125_RED
NASA/JPL-Caltech/University of Arizona
This feature was first viewed by the CaSSIS instrument, and is similar to the ones in Nili Fossae. An inverted channel?
https://www.uahirise.org/anaglyph/ESP_089248_2125_ESP_078541_2125_RED
NASA/JPL-Caltech/University of Arizona
Relatively dark slope streaks are common on steep dust-mantled slopes of Mars. At high resolution), we can clearly see that surface material has been removed from the upper slopes as expected from landslides.
More: https://uahirise.org/hipod/ESP_067900_1935
Relatively dark slope streaks are common on steep dust-mantled slopes of Mars. At high resolution), we can clearly see that surface material has been removed from the upper slopes as expected from landslides.
More: https://uahirise.org/hipod/ESP_067900_1935
Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. These dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide.
https://uahirise.org/hipod/ESP_045311_1205
#Mars #science #NASA
Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. These dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide.
https://uahirise.org/hipod/ESP_045311_1205
#Mars #science #NASA
My God, it’s full
of stars.
My God, it’s full
of stars.