Phobos (Estonian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Phobos" in Estonian language version.

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aas.org (Global: 9,251st place; Estonian: low place)

adsabs.harvard.edu (Global: 14th place; Estonian: 71st place)

ui.adsabs.harvard.edu

archive.org (Global: 6th place; Estonian: 17th place)

bbc.co.uk (Global: 11th place; Estonian: 41st place)

doi.org (Global: 2nd place; Estonian: 8th place)

esa.int (Global: 1,073rd place; Estonian: 238th place)

sci.esa.int

nasa.gov (Global: 12th place; Estonian: 47th place)

solarsystem.nasa.gov

physorg.com (Global: 8,229th place; Estonian: 2,735th place)

solarviews.com (Global: low place; Estonian: 2,330th place)

  • "Stickney Crater-Phobos". One of the most striking features of Phobos, aside from its irregular shape, is its giant crater Stickney. Because Phobos is only Mall:Convert, the moon must have been nearly shattered from the force of the impact that caused the giant crater. Grooves that extend across the surface from Stickney appear to be surface fractures caused by the impact.

space.com (Global: 862nd place; Estonian: 149th place)

umd.edu (Global: 1,356th place; Estonian: 2,362nd place)

astro.umd.edu

usgs.gov (Global: 119th place; Estonian: 226th place)

planetarynames.wr.usgs.gov

usra.edu (Global: 1,836th place; Estonian: 2,290th place)

lpi.usra.edu

  • Murray, J. B.; et al. "New Evidence on the Origin of Phobos' Parallel Grooves from HRSC Mars Express" (PDF). 37th Annual Lunar and Planetary Science Conference, March 2006. {{cite web}}: et al.-i üleliigne kasutus kohas: |author= (juhend)
  • Ivanov, Andrei; Zolensky, Michael (2003). "The Kaidun Meteorite: Where Did It Come From?" (PDF). Lunar and Planetary Science. 34. The currently available data on the lithologic composition of the Kaidun meteorite– primarily the composition of the main portion of the meteorite, corresponding to CR2 carbonaceous chondrites and the presence of clasts of deeply differentiated rock – provide weighty support for considering the meteorite’s parent body to be a carbonaceous chondrite satellite of a large differentiated planet. The only possible candidates in the modern solar system are Phobos and Deimos, the moons of Mars.

web.archive.org (Global: 1st place; Estonian: 1st place)

worldcat.org (Global: 4th place; Estonian: 18th place)