Phobos (Estonian Wikipedia)

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

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7harvard.edu

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2nasa.gov

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aas.org

"Porosity of Small Bodies and a Reassesment of Ida's Density". Originaali arhiivikoopia seisuga 26. september 2007. Vaadatud 5. aprillil 2014. When the error bars are taken into account, only one of these, Phobos, has a porosity below 0.2...

archive.org

Lewis, J. S. (2004). Physics and Chemistry of the Solar System. Elsevier Academic Press. Lk 425. ISBN 0-12-446744-X.

bbc.co.uk

"Phobos".

doi.org

Busch, M. W. (2007). "Arecibo Radar Observations of Phobos and Deimos". Icarus. 186 (2): 581–584. Bibcode:2007Icar..186..581B. DOI:10.1016/j.icarus.2006.11.003. ISSN 0019-1035.
Rivkin, A. S. (märts 2002). "Near-Infrared Spectrophotometry of Phobos and Deimos". Icarus. 156 (1): 64. Bibcode:2002Icar..156...64R. DOI:10.1006/icar.2001.6767.
Fanale, F. P.; Salvail, J. R. (1989). "Loss of water from Phobos". Geophys. Res. Lett. 16: 287–290. Bibcode:1989GeoRL..16..287F. DOI:10.1029/GL016i004p00287.
Fanale, Fraser P.; Salvail, James R. (detsember 1990). "Evolution of the water regime of Phobos". Icarus. 88: 380–395. Bibcode:1990Icar...88..380F. DOI:10.1016/0019-1035(90)90089-R.
Showalter, M. R.; Hamilton, D. P. and Nicholson, P. D. (2006). "A Deep Search for Martian Dust Rings and Inner Moons Using the Hubble Space Telescope" (PDF). Planetary and Space Science. 54 (9–10): 844–854. Bibcode:2006P&SS...54..844S. DOI:10.1016/j.pss.2006.05.009.{{cite journal}}: CS1 hooldus: mitu nime: autorite loend (link)
Ivanov, Andrei V. (märts 2004). "Is the Kaidun Meteorite a Sample from Phobos?". Solar System Research. 38 (2): 97–107. Bibcode:2004SoSyR..38...97I. DOI:10.1023/B:SOLS.0000022821.22821.84.

esa.int

sci.esa.int

"Close Inspection for Phobos". It is light, with a density less than twice that of water, and orbits just Mall:Convert above the Martian surface.

harvard.edu

ui.adsabs.harvard.edu

Busch, M. W. (2007). "Arecibo Radar Observations of Phobos and Deimos". Icarus. 186 (2): 581–584. Bibcode:2007Icar..186..581B. DOI:10.1016/j.icarus.2006.11.003. ISSN 0019-1035.
Murchie, S. L.; Erard, S., Langevin, Y., Britt, D. T., Bibring, J. P., and Mustard, J. F. (1991). "Disk-resolved Spectral Reflectance Properties of Phobos from 0.3-3.2 microns: Preliminary Integrated Results from PhobosH 2". Abstracts of the Lunar and Planetary Science Conference. 22: 943. Bibcode:1991pggp.rept..249M.{{cite journal}}: CS1 hooldus: mitu nime: autorite loend (link)
Rivkin, A. S. (märts 2002). "Near-Infrared Spectrophotometry of Phobos and Deimos". Icarus. 156 (1): 64. Bibcode:2002Icar..156...64R. DOI:10.1006/icar.2001.6767.
Fanale, F. P.; Salvail, J. R. (1989). "Loss of water from Phobos". Geophys. Res. Lett. 16: 287–290. Bibcode:1989GeoRL..16..287F. DOI:10.1029/GL016i004p00287.
Fanale, Fraser P.; Salvail, James R. (detsember 1990). "Evolution of the water regime of Phobos". Icarus. 88: 380–395. Bibcode:1990Icar...88..380F. DOI:10.1016/0019-1035(90)90089-R.
Showalter, M. R.; Hamilton, D. P. and Nicholson, P. D. (2006). "A Deep Search for Martian Dust Rings and Inner Moons Using the Hubble Space Telescope" (PDF). Planetary and Space Science. 54 (9–10): 844–854. Bibcode:2006P&SS...54..844S. DOI:10.1016/j.pss.2006.05.009.{{cite journal}}: CS1 hooldus: mitu nime: autorite loend (link)
Ivanov, Andrei V. (märts 2004). "Is the Kaidun Meteorite a Sample from Phobos?". Solar System Research. 38 (2): 97–107. Bibcode:2004SoSyR..38...97I. DOI:10.1023/B:SOLS.0000022821.22821.84.

nasa.gov

solarsystem.nasa.gov

"NASA - Phobos". Originaali arhiivikoopia seisuga 24. juuni 2014. Vaadatud 5. aprillil 2014.
"Solar System Exploration: Planets: Mars: Moons: Phobos: Overview". Solarsystem.nasa.gov. Originaali arhiivikoopia seisuga 24. juuni 2014. Vaadatud 19. augustil 2013.

physorg.com

"New Views of Martian Moons".

solarviews.com

"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

Britt, Robert Roy (13. märts 2001). "Forgotten Moons: Phobos and Deimos Eat Mars' Dust". space.com. Originaali arhiivikoopia seisuga 19.06.2001. Vaadatud 12. mail 2010.

umd.edu

astro.umd.edu

Showalter, M. R.; Hamilton, D. P. and Nicholson, P. D. (2006). "A Deep Search for Martian Dust Rings and Inner Moons Using the Hubble Space Telescope" (PDF). Planetary and Space Science. 54 (9–10): 844–854. Bibcode:2006P&SS...54..844S. DOI:10.1016/j.pss.2006.05.009.{{cite journal}}: CS1 hooldus: mitu nime: autorite loend (link)

usgs.gov

planetarynames.wr.usgs.gov

usra.edu

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

"NASA - Phobos". Originaali arhiivikoopia seisuga 24. juuni 2014. Vaadatud 5. aprillil 2014.
Mars: Moons: Phobos, NASA Solar System Exploration, 30. september 2003
"Solar System Exploration: Planets: Mars: Moons: Phobos: Overview". Solarsystem.nasa.gov. Originaali arhiivikoopia seisuga 24. juuni 2014. Vaadatud 19. augustil 2013.
"Porosity of Small Bodies and a Reassesment of Ida's Density". Originaali arhiivikoopia seisuga 26. september 2007. Vaadatud 5. aprillil 2014. When the error bars are taken into account, only one of these, Phobos, has a porosity below 0.2...
Britt, Robert Roy (13. märts 2001). "Forgotten Moons: Phobos and Deimos Eat Mars' Dust". space.com. Originaali arhiivikoopia seisuga 19.06.2001. Vaadatud 12. mail 2010.

worldcat.org

Busch, M. W. (2007). "Arecibo Radar Observations of Phobos and Deimos". Icarus. 186 (2): 581–584. Bibcode:2007Icar..186..581B. DOI:10.1016/j.icarus.2006.11.003. ISSN 0019-1035.