溝槽和紋理

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參考資料

1. ^^1.01.11.2Planetary Names: Crater, craters: Stickney on Phobos. Gazetteer of Planetary Nomenclature. 2006-11-29 [2020-10-11]. （原始内容存档于2020-10-14）. 
2. ^"Stickney".Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
3. ^Hall, Asaph,Observations and orbits of the satellites of Mars, Washington: Government Printing Office, 1878 (quoted in Hall, Angelo,An astronomer's wife, Baltimore: Nunn and Company, 1908, p. 112).
4. ^Veverka, Joseph et al. "A Mariner 9 atlas of the moons of Mars,"Icarus 23, 206-289 (1974).
5. ^Calculating theangular size of an object with a diameter of 9km at a distance of 9250km, yields 9/9250 * 206265 = 200 arcseconds. An object needs a size of 60 arcseconds to be resolved by thenaked eye.
6. ^Murray, John B. et al. "New evidence on the origin of Phobos' parallel grooves from HRSC Mars Express （页面存档备份，存于互联网档案馆）," Lunar and Planetary Science XXXVII (2006).
7. ^Zubritsky, Elizabeth.Mars' Moon Phobos is Slowly Falling Apart. NASA's Goddard Space Flight Center. 2015-11-10 [11 November 2015]. （原始内容存档于2019-07-27）. 
8. ^^8.08.1Gough, Evan.Strange Grooves on Phobos Were Caused by Boulders Rolling Around on its Surface.Universe Today. 20 November 2018 [21 November 2018]. （原始内容存档于2019-07-31）. 
9. ^Ramsley, Kenneth R.; Head, James W. Origin of Phobos grooves: Testing the Stickney Crater ejecta model.Planetary and Space Science. 16 November 2018,165: 137–147.doi:10.1016/j.pss.2018.11.004. 
10. ^Phobos from 6,800 Kilometers (Color). NASA/JPL-Caltech/University of Arizona. 2008-04-09 [2008-04-09]. （原始内容存档于2008-04-12）. 

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