Difference between revisions of "The beauty of Mars from 150 miles"
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[[File:Brain terrain from around Mars 02.jpg|600pxr| Image shows the variety of different kinds of brain terrain on Mars. Brain terrain is called that because it resembles the surface of the human brain. It is thought to form when ice leaves the ground along cracks. ]] | [[File:Brain terrain from around Mars 02.jpg|600pxr| Image shows the variety of different kinds of brain terrain on Mars. Brain terrain is called that because it resembles the surface of the human brain. It is thought to form when ice leaves the ground along cracks. ]] | ||
| − | Image shows the variety of different kinds of brain terrain on Mars. Brain terrain is called that because it resembles the surface of the human brain. It is thought to form when ice leaves the ground along cracks. | + | Image shows the variety of different kinds of brain terrain on Mars. Brain terrain is called that because it resembles the surface of the human brain. It is thought to form when ice leaves the ground along cracks.<ref name=":0">Levy, J., J. Head, D. Marchant. 2009. Concentric crater fill in Utopia Planitia: History and interaction between glacial “brain terrain” and periglacial mantle processes. Icarus 202, 462–476.</ref> <ref name="Baker, D. 2015">Baker, D., J. Head. 2015. Extensive Middle Amazonian mantling of debris aprons and plains in Deuteronilus Mensae, Mars: Implication for the record of mid-latitude glaciation. Icarus: 260, 269-288.</ref> |
Revision as of 15:50, 25 November 2023
Article written by Jim Secosky. Jim is a retired science teacher who has used the Hubble Space Telescope, the Mars Global Surveyor, and HiRISE.
This article will show some beautiful scenes of Mars from about 150 miles above the surface. The pictures were taken by the High Resolution Imaging Science Experiment (HiRISE) that orbits Mars. The colors are from a central strip in each of the images. The colors are processed to bring out more information about the minerals on the surface. ; they are not exactly what we would see with just our eyes. Some incorporate an infrared band which humans can't see.
The pictures are a labor of love for Jim Secosky. He started suggesting places for NASA to observe in 2010 through the HiWish program. Every one of the pictures here were ones that he obtained through the HiWish program. that program allows anyone to explore Mars. However, one often has to wait months or years for the pictures to be taken, processed, and released. The satellite mostly just takes pictures of what it passes over; hence, you may have to wait until it passes over something you suggested.
A few of the images have a box--that box represents the size of a football field (100 yards).
The collections of pictures here will not include much geology. If you want to find out more, you can go to the references or links to other articles in Marspedia. Some talks are also listed that Jim gave for the Mars Society.
Collage of pictures taken with HiRISE under HiWish program
Image shows the variety of different kinds of brain terrain on Mars. Brain terrain is called that because it resembles the surface of the human brain. It is thought to form when ice leaves the ground along cracks.[1] [2]
Different kinds of impact craters on Mars.
Image shows dust devil tracks on Mars. Mars has many dust devils. When a dust devil passes, it removes the thin coating of bright dust. One then sees the dark undersurface.
Image shows the variety of channels on Mars. In the past Mars once had many streams and rivers.
Glaciers on Mars. Some have ice; some have lost most of their ice. The ice was able to be preserved for long periods because it had a layer of dirt and rocks on top.
Sand dunes on Mars. The colored ones are from a colored strip in the center of each HiRISE image. To our eyes all of these would probably appear black. However, NASA images are able to be processed to bring out slight differences. Dunes are made of the black volcanic rock basalt. Basalt does not always have the same exact composition. Slight amounts of certain elements can yield slightly different colors.
Image shows the variety of mud volcanoes on Mars. The mud comes up from a distance such that organisms could have lived in the mud. On the surface living things were die from the radiation. The colored ones are from a colored strip in the center of each HiRISE image.
Ridges on Mars. Ridges sometimes form shapes at nearly right angles. We do not know the exact cause, but a popular idea is that minerals were deposited in cracks.[3] Later, erosion removed the soft material around them. There is some evidence that clays are near them. That's important because clays need water to form. Hence, they may be markers of past water. The colored ones are from a colored strip in the center of each HiRISE image.
Streamlined forms on Mars. Great floods formed these. Nearness to volcanic features or maybe an impact may have released water from the frozen ground. The colored ones are from a colored strip in the center of each HiRISE image.
Gullies on Mars. Gullies from on steep slopes. Today, they seem to be produced with the action of dry ice; in the past liquid water may have been involved. The colored ones are from a colored strip in the center of each HiRISE image.
Landslides on Mars
Troughs on Mars. Troughs form on Mars due to the huge volcanoes weighing down the crust and stretching it.
Shapes observed on floor of Hellas. The shapes are strange and we currently do not know exactly how they were formed. Glaciers may have been involved.
Hollows on Mars. Hollows are produced when ice leaves the ground.
Lava flows on Mars
Scalloped terrain on Mars. This terrain forms when ice leaves the ground. It is a marker for ice.
Rootless cones on Mars. They form when lava flows over frozen or ice-rich ground.
Layered hills on Mars. They are the remains of material that once covered a wide area.
Plumes and spiders on Mars In the spring, black dust/sand blows out of the ground and makes dark plumes. Plumes may elongated shapes due to the wind. Some shapes that look like spiders are created.
Dark slope streaks on Mars. Most believe they are avalanches of bright dust.
Volcanic vents on Mars.
Common features seen on Mars
Layered landscapes of Mars
See Also
- Geography of Mars
- Glaciers on Mars
- High Resolution Imaging Science Experiment (HiRISE)
- Layers on Mars
- Martian features that are signs of water ice
- Martian gullies
- Rivers on Mars
- Sublimation
- Sublimation landscapes on Mars
External links
- https://planetarynames.wr.usgs.gov/Page/MARS/target For information on names and locations on Mars
- Seeing the wonders of Mars with HiRISE under the HiWish program
- Features of Mars with HiRISE under HiWish program Shows nearly all major features discovered on Mars. This would be good for teachers covering Mars.
- Martian Ice - Jim Secosky - 16th Annual International Mars Society Convention
- Martian Geology - Jim Secosky - 16th Annual International Mars Society Convention
- Walks on Mars - Jim Secosky - 16th Annual International Mars Society Convention
References
- ↑ Levy, J., J. Head, D. Marchant. 2009. Concentric crater fill in Utopia Planitia: History and interaction between glacial “brain terrain” and periglacial mantle processes. Icarus 202, 462–476.
- ↑ Baker, D., J. Head. 2015. Extensive Middle Amazonian mantling of debris aprons and plains in Deuteronilus Mensae, Mars: Implication for the record of mid-latitude glaciation. Icarus: 260, 269-288.
- ↑ Saper, L., J. Mustard. 2013. "Extensive linear ridge networks in Nili Fossae and Nilosyrtis, Mars: implications for fluid flow in the ancient crust". Geophysical Research Letters: 40, 245-249.
