靈神星 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "靈神星" in Chinese language version.

refsWebsite

Global rank Chinese rank

8harvard.edu

18^th place

57^th place

7web.archive.org

1^st place

6doi.org

2^nd place

23^rd place

2semanticscholar.org

11^th place

332^nd place

2arxiv.org

69^th place

254^th place

1nasa.gov

75^th place

140^th place

1webcitation.org

24^th place

29^th place

1earthlink.net

7,693^rd place

low place

1psi.edu

low place

1navy.mil

237^th place

329^th place

1earthsky.org

6,724^th place

low place

1helsinki.fi

1,670^th place

3,212^th place

arxiv.org

Johnson, B.C.; Sori, M.M.; Evans, A.J. Ferrovolcanism of metal worlds and the origin of pallasites. Nature Astronomy. 2020, 4: 41–44. Bibcode:2020NatAs...4...41J. S2CID 202583406. arXiv:1909.07451 . doi:10.1038/s41550-019-0885-x.
Shepard, Michael K.; De Kleer, Katherine; Cambioni, Saverio; Taylor, Patrick A.; Virkki, Anne K.; Rívera-Valentin, Edgard G.; Rodriguez Sanchez-Vahamonde, Carolina; Fernanda Zambrano-Marin, Luisa; Magri, Christopher; Dunham, David; Moore, John; Camarca, Maria. Asteroid 16 Psyche: Shape, Features, and Global Map. The Planetary Science Journal. 2021, 2 (4): 125. Bibcode:2021PSJ.....2..125S. S2CID 235918955. arXiv:2110.03635 . doi:10.3847/PSJ/abfdba .

doi.org

Lupishko, D. F. On the bulk density and porosity of M-type asteroid 16 Psyche. Solar System Research. 2006, 40 (3): 214–218. Bibcode:2006SoSyR..40..214L. doi:10.1134/S0038094606030051.
Asphaug, E.; Reufer, A. Mercury and other iron-rich planetary bodies as relics of inefficient accretion. Nature Geoscience. 2014, 7 (8): 564–568. Bibcode:2014NatGe...7..564A. doi:10.1038/NGEO2189.
Davis, D.R.; Farinella, Paolo & Francesco, M. The missing Psyche family: Collisionally eroded or never formed?. Icarus. 1999, 137 (1): 140. Bibcode:1999Icar..137..140D. doi:10.1006/icar.1998.6037.
Johnson, B.C.; Sori, M.M.; Evans, A.J. Ferrovolcanism of metal worlds and the origin of pallasites. Nature Astronomy. 2020, 4: 41–44. Bibcode:2020NatAs...4...41J. S2CID 202583406. arXiv:1909.07451 . doi:10.1038/s41550-019-0885-x.
Shepard, Michael K.; De Kleer, Katherine; Cambioni, Saverio; Taylor, Patrick A.; Virkki, Anne K.; Rívera-Valentin, Edgard G.; Rodriguez Sanchez-Vahamonde, Carolina; Fernanda Zambrano-Marin, Luisa; Magri, Christopher; Dunham, David; Moore, John; Camarca, Maria. Asteroid 16 Psyche: Shape, Features, and Global Map. The Planetary Science Journal. 2021, 2 (4): 125. Bibcode:2021PSJ.....2..125S. S2CID 235918955. arXiv:2110.03635 . doi:10.3847/PSJ/abfdba .
M. Kaasalainen; et al. Models of Twenty Asteroids from Photometric Data (PDF). Icarus. 2002, 159 (2): 369 [16 May 2006]. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907. （原始内容存档 (PDF)于2015-11-05）.

earthlink.net

home.earthlink.net

Jim Baer. Recent Asteroid Mass Determinations. Personal Website. 2008 [2008-12-04]. （原始内容存档于2013-07-08）.

earthsky.org

Kelly Kizer Whitt. Asteroid Psyche: $10,000 quadrillion or rubble pile?. EarthSky. 2021-06-16 [2022-02-28]. （原始内容存档于2021-11-21）.

harvard.edu

ui.adsabs.harvard.edu

Lupishko, D. F. On the bulk density and porosity of M-type asteroid 16 Psyche. Solar System Research. 2006, 40 (3): 214–218. Bibcode:2006SoSyR..40..214L. doi:10.1134/S0038094606030051.
Asphaug, E.; Reufer, A. Mercury and other iron-rich planetary bodies as relics of inefficient accretion. Nature Geoscience. 2014, 7 (8): 564–568. Bibcode:2014NatGe...7..564A. doi:10.1038/NGEO2189.
Davis, D.R.; Farinella, Paolo & Francesco, M. The missing Psyche family: Collisionally eroded or never formed?. Icarus. 1999, 137 (1): 140. Bibcode:1999Icar..137..140D. doi:10.1006/icar.1998.6037.
Johnson, B.C.; Sori, M.M.; Evans, A.J. Ferrovolcanism of metal worlds and the origin of pallasites. Nature Astronomy. 2020, 4: 41–44. Bibcode:2020NatAs...4...41J. S2CID 202583406. arXiv:1909.07451 . doi:10.1038/s41550-019-0885-x.
Shepard, Michael K.; De Kleer, Katherine; Cambioni, Saverio; Taylor, Patrick A.; Virkki, Anne K.; Rívera-Valentin, Edgard G.; Rodriguez Sanchez-Vahamonde, Carolina; Fernanda Zambrano-Marin, Luisa; Magri, Christopher; Dunham, David; Moore, John; Camarca, Maria. Asteroid 16 Psyche: Shape, Features, and Global Map. The Planetary Science Journal. 2021, 2 (4): 125. Bibcode:2021PSJ.....2..125S. S2CID 235918955. arXiv:2110.03635 . doi:10.3847/PSJ/abfdba .
M. Kaasalainen; et al. Models of Twenty Asteroids from Photometric Data (PDF). Icarus. 2002, 159 (2): 369 [16 May 2006]. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907. （原始内容存档 (PDF)于2015-11-05）.

articles.adsabs.harvard.edu

S.J. Ostro. Radar observations of asteroids and comets (PDF). Astronomical Society of the Pacific, Publications. 1985, 97: 877 [2019-04-06]. （原始内容存档 (PDF)于2016-06-12）.

adsabs.harvard.edu

P.S. Hardersen, M.J. Gaffey, and P.A. Abell. Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids. Icarus. 2005, 175: 141 [2019-04-06]. （原始内容存档于2016-06-12）.

helsinki.fi

rni.helsinki.fi

M. Kaasalainen; et al. Models of Twenty Asteroids from Photometric Data (PDF). Icarus. 2002, 159 (2): 369 [16 May 2006]. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907. （原始内容存档 (PDF)于2015-11-05）.

nasa.gov

ssd.jpl.nasa.gov

JPL Small-Body Database Browser: 16 Psyche. 2008-09-19 [2008-12-04]. （原始内容存档于2020-07-24）.

navy.mil

aa.usno.navy.mil

Hilton, J. When Did the Asteroids Become Minor Planets?. U.S. Naval Observatory. September 17, 2001 [2007-04-03]. （原始内容存档于2006-05-20）.

psi.edu

PDS lightcurve data. [2007-08-29]. （原始内容存档于2016-03-04）.

semanticscholar.org

api.semanticscholar.org

Johnson, B.C.; Sori, M.M.; Evans, A.J. Ferrovolcanism of metal worlds and the origin of pallasites. Nature Astronomy. 2020, 4: 41–44. Bibcode:2020NatAs...4...41J. S2CID 202583406. arXiv:1909.07451 . doi:10.1038/s41550-019-0885-x.
Shepard, Michael K.; De Kleer, Katherine; Cambioni, Saverio; Taylor, Patrick A.; Virkki, Anne K.; Rívera-Valentin, Edgard G.; Rodriguez Sanchez-Vahamonde, Carolina; Fernanda Zambrano-Marin, Luisa; Magri, Christopher; Dunham, David; Moore, John; Camarca, Maria. Asteroid 16 Psyche: Shape, Features, and Global Map. The Planetary Science Journal. 2021, 2 (4): 125. Bibcode:2021PSJ.....2..125S. S2CID 235918955. arXiv:2110.03635 . doi:10.3847/PSJ/abfdba .

web.archive.org

JPL Small-Body Database Browser: 16 Psyche. 2008-09-19 [2008-12-04]. （原始内容存档于2020-07-24）.
PDS lightcurve data. [2007-08-29]. （原始内容存档于2016-03-04）.
Hilton, J. When Did the Asteroids Become Minor Planets?. U.S. Naval Observatory. September 17, 2001 [2007-04-03]. （原始内容存档于2006-05-20）.
S.J. Ostro. Radar observations of asteroids and comets (PDF). Astronomical Society of the Pacific, Publications. 1985, 97: 877 [2019-04-06]. （原始内容存档 (PDF)于2016-06-12）.
P.S. Hardersen, M.J. Gaffey, and P.A. Abell. Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids. Icarus. 2005, 175: 141 [2019-04-06]. （原始内容存档于2016-06-12）.
Kelly Kizer Whitt. Asteroid Psyche: $10,000 quadrillion or rubble pile?. EarthSky. 2021-06-16 [2022-02-28]. （原始内容存档于2021-11-21）.
M. Kaasalainen; et al. Models of Twenty Asteroids from Photometric Data (PDF). Icarus. 2002, 159 (2): 369 [16 May 2006]. Bibcode:2002Icar..159..369K. doi:10.1006/icar.2002.6907. （原始内容存档 (PDF)于2015-11-05）.

webcitation.org

Jim Baer. Recent Asteroid Mass Determinations. Personal Website. 2008 [2008-12-04]. （原始内容存档于2013-07-08）.