MESSENGER image with Chesterton at left | |
| Feature type | Impact crater |
|---|---|
| Location | Borealis quadrangle, Mercury |
| Coordinates | 88°31′N 126°54′W / 88.51°N 126.9°W |
| Diameter | 37.23 km |
| Eponym | Gilbert Keith Chesterton |
Chesterton is a crater on Mercury, near the north pole. Its name was adopted by the International Astronomical Union in 2012, after the English author G. K. Chesterton. [1]
The floor of the crater is in permanent shadow. S band radar data from the Arecibo Observatory collected between 1999 and 2005 indicates a radar-bright area covering the entire floor of Chesterton, which is probably indicative of a water ice deposit. [2] [3] [4]
Chesterton is adjacent to Tryggvadóttir crater.
References
- ^ "Chesterton". Gazetteer of Planetary Nomenclature. NASA. Retrieved 23 March 2020.
- ^ Chabot, N. L., D. J. Lawrence, G. A. Neumann, W. C. Feldman, and D. A. Paige, 2018. Mercury's Polar Deposits. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 13, Figure 13.2.
- ^ PIA19411: Water Ice on Mercury, NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
- ^ John K. Harmon, Martin A. Slade, Melissa S. Rice, 2011. Radar imagery of Mercury’s putative polar ice: 1999–2005 Arecibo results. Icarus, 211, p37-50. doi.org/10.1016/j.icarus.2010.08.007
 | This article about the planet Mercury is a stub. You can help Wikipedia by expanding it. |
|
MESSENGER image with Chesterton at left | |
| Feature type | Impact crater |
|---|---|
| Location | Borealis quadrangle, Mercury |
| Coordinates | 88°31′N 126°54′W / 88.51°N 126.9°W |
| Diameter | 37.23 km |
| Eponym | Gilbert Keith Chesterton |
Chesterton is a crater on Mercury, near the north pole. Its name was adopted by the International Astronomical Union in 2012, after the English author G. K. Chesterton. [1]
The floor of the crater is in permanent shadow. S band radar data from the Arecibo Observatory collected between 1999 and 2005 indicates a radar-bright area covering the entire floor of Chesterton, which is probably indicative of a water ice deposit. [2] [3] [4]
Chesterton is adjacent to Tryggvadóttir crater.
References
- ^ "Chesterton". Gazetteer of Planetary Nomenclature. NASA. Retrieved 23 March 2020.
- ^ Chabot, N. L., D. J. Lawrence, G. A. Neumann, W. C. Feldman, and D. A. Paige, 2018. Mercury's Polar Deposits. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 13, Figure 13.2.
- ^ PIA19411: Water Ice on Mercury, NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
- ^ John K. Harmon, Martin A. Slade, Melissa S. Rice, 2011. Radar imagery of Mercury’s putative polar ice: 1999–2005 Arecibo results. Icarus, 211, p37-50. doi.org/10.1016/j.icarus.2010.08.007
|
| This article about the planet Mercury is a stub. You can help Wikipedia by expanding it. |