M-type asteroid (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "M-type asteroid" in English language version.

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20doi.org

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14semanticscholar.org

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9harvard.edu

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7arxiv.org

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5nih.gov

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3nasa.gov

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2handle.net

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1mit.edu

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1aanda.org

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aanda.org

Marchis, F.; Jorda, L.; Vernazza, P.; Brož, M.; Hanuš, J.; Ferrais, M.; et al. (September 2021). "(216) Kleopatra, a low density, critically rotating, M-type asteroid". Astronomy & Astrophysics. 653: A57. arXiv:2108.07207. doi:10.1051/0004-6361/202140874. S2CID 237091036. A57. Retrieved 13 October 2021.

arxiv.org

Pitjeva, E.V.; Pitjev, N.P. (2018). "Masses of the main asteroid belt and the Kuiper belt from the motions of planets and spacecraft". Earth and Planetary Astrophysics. 44 (8–9): 554–566. arXiv:1811.05191v1. doi:10.1134/S1063773718090050. S2CID 255197841.
Shepard, M.K.; et al. (2021). "Asteroid 16 Psyche: Shape, features, and global map". The Planetary Science Journal. 2 (4): 16. arXiv:2110.03635. doi:10.3847/PSJ/abfdba. S2CID 235918955.
Carry, B. (2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.
Marchis, F.; Jorda, L.; Vernazza, P.; Brož, M.; Hanuš, J.; Ferrais, M.; et al. (September 2021). "(216) Kleopatra, a low density, critically rotating, M-type asteroid". Astronomy & Astrophysics. 653: A57. arXiv:2108.07207. doi:10.1051/0004-6361/202140874. S2CID 237091036. A57. Retrieved 13 October 2021.
Descamps, P.; Marchis, F.; Pollock, J.; Berthier, J.; Vachier, F.; Birlan, M.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. S2CID 118437111.
Johnson, B.C.; Sori, M.M.; Evans, A.J. (2020). "Ferrovolcanism of metal worlds and the origin of pallasites". Nature Astronomy. 4: 41–44. arXiv:1909.07451. doi:10.1038/s41550-019-0885-x. S2CID 202583406.
Descamps, P.; et al. (2011). "Triplicity and physical characteristics of asteroid (216) Kleopatra". Icarus. 245 (2): 64–69. arXiv:1011.5263. doi:10.1016/j.icarus.2010.11.016. S2CID 119286272.

doi.org

Shepard, M.K.; et al. (2015). "A radar survey of M- and X-class asteroids: III. Insights into their composition, hydration state, and structure". Icarus. 245: 38–55. doi:10.1016/j.icarus.2014.09.016.
Magri, C.; et al. (2007). "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999–2004". Icarus. 186: 126–151. doi:10.1016/j.icarus.2006.08.018.
Bus, S.J.; Binzel, R.P. (2002). "Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy". Icarus. 158 (1): 146–177. Bibcode:2002Icar..158..146B. doi:10.1006/icar.2002.6856. S2CID 4880578.
Ockert-Bell, M.; et al. (2010). "The composition of M-type asteroids: Synthesis of spectroscopic and radar observations". Icarus. 210 (2): 674–692. doi:10.1016/j.icarus.2010.08.002.
Rivkin, A.S.; et al. (2000). "The nature of M-class asteroids from 3-micron observations". Icarus. 145 (2): 351. Bibcode:2000Icar..145..351R. doi:10.1006/icar.2000.6354.
Pitjeva, E.V.; Pitjev, N.P. (2018). "Masses of the main asteroid belt and the Kuiper belt from the motions of planets and spacecraft". Earth and Planetary Astrophysics. 44 (8–9): 554–566. arXiv:1811.05191v1. doi:10.1134/S1063773718090050. S2CID 255197841.
Elkins-Tanton, L. T.; et al. (2020). "Observations, meteorites, and models: A preflight assessment of the composition and formation of (16) Psyche". Journal of Geophysical Research: Planets. 125 (3): 23. doi:10.1029/2019JE006296. PMC 7375145. PMID 32714727. S2CID 214018872.
Shepard, M.K.; et al. (2021). "Asteroid 16 Psyche: Shape, features, and global map". The Planetary Science Journal. 2 (4): 16. arXiv:2110.03635. doi:10.3847/PSJ/abfdba. S2CID 235918955.
Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.
Vernazza, P.; et al. (2021). "VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis". Astronomy and Astrophysics. 654 (A56): 48. doi:10.1051/0004-6361/202141781. hdl:10261/263281. S2CID 239104699.
Carry, B. (2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.
Marchis, F.; Jorda, L.; Vernazza, P.; Brož, M.; Hanuš, J.; Ferrais, M.; et al. (September 2021). "(216) Kleopatra, a low density, critically rotating, M-type asteroid". Astronomy & Astrophysics. 653: A57. arXiv:2108.07207. doi:10.1051/0004-6361/202140874. S2CID 237091036. A57. Retrieved 13 October 2021.
Shepard, Michael K.; Timerson, Bradley; Scheeres, Daniel J.; Benner, Lance A.M.; Giorgini, Jon D.; Howell, Ellen S.; et al. (2018). "A revised shape model of asteroid (216) Kleopatra". Icarus. 311: 197–209. Bibcode:2018Icar..311..197S. doi:10.1016/j.icarus.2018.04.002.
Descamps, P.; Marchis, F.; Pollock, J.; Berthier, J.; Vachier, F.; Birlan, M.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. S2CID 118437111.
Davis, D.R.; Farinella, P.; Marzari, F. (1999). "The missing Psyche family: Collisionally eroded or never formed?". Icarus. 137 (1): 140–151. doi:10.1006/icar.1998.6037.
Johnson, B.C.; Sori, M.M.; Evans, A.J. (2020). "Ferrovolcanism of metal worlds and the origin of pallasites". Nature Astronomy. 4: 41–44. arXiv:1909.07451. doi:10.1038/s41550-019-0885-x. S2CID 202583406.
Schulz, R.; et al. (2012). "Rosetta fly-by at asteroid (21) Lutetia: An overview". Planetary and Space Science. 66 (1): 2–8. doi:10.1016/j.pss.2011.11.013.
Coradini, A.; et al. (2011). "The surface composition and temperature of asteroid 21 Lutetia as observed by Rosetta/VIRTIS". Science. 334 (492): 492–494. doi:10.1126/science.1204062. PMID 22034430. S2CID 19439721.
Margot, J.L.; Brown, M.E. (2003). "A low-density M-type asteroid in the main belt". Science. 300 (5627): 1939–1942. doi:10.1126/science.1085844. PMID 12817147. S2CID 5479442.
Descamps, P.; et al. (2011). "Triplicity and physical characteristics of asteroid (216) Kleopatra". Icarus. 245 (2): 64–69. arXiv:1011.5263. doi:10.1016/j.icarus.2010.11.016. S2CID 119286272.

handle.net

hdl.handle.net

Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.
Vernazza, P.; et al. (2021). "VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis". Astronomy and Astrophysics. 654 (A56): 48. doi:10.1051/0004-6361/202141781. hdl:10261/263281. S2CID 239104699.

harvard.edu

ui.adsabs.harvard.edu

Bus, S.J.; Binzel, R.P. (2002). "Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy". Icarus. 158 (1): 146–177. Bibcode:2002Icar..158..146B. doi:10.1006/icar.2002.6856. S2CID 4880578.
Lupishko, D.F.; et al. (1982). "UBV photometry of the M-type asteroids 16 Psyche and 22 Kalliope". Solar System Research. 16: 75. Bibcode:1982AVest..16..101L.
Rivkin, A.S.; et al. (2000). "The nature of M-class asteroids from 3-micron observations". Icarus. 145 (2): 351. Bibcode:2000Icar..145..351R. doi:10.1006/icar.2000.6354.
Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.
Ferrais, M. (2021). M-type (22) Kalliope: High density and differentiated interior. 15th Europlanet Science Congress. Bibcode:2021EPSC...15..696F. Retrieved 30 December 2021 – via NASA ADS.
Shepard, Michael K.; Timerson, Bradley; Scheeres, Daniel J.; Benner, Lance A.M.; Giorgini, Jon D.; Howell, Ellen S.; et al. (2018). "A revised shape model of asteroid (216) Kleopatra". Icarus. 311: 197–209. Bibcode:2018Icar..311..197S. doi:10.1016/j.icarus.2018.04.002.
Descamps, P.; Marchis, F.; Pollock, J.; Berthier, J.; Vachier, F.; Birlan, M.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. S2CID 118437111.
Scott, E.; et al. (2014). "Origin of igneous meteorites and differentiated asteroids". Asteroids. ACM: 483. Bibcode:2014acm..conf..483S.

articles.adsabs.harvard.edu

Scott, E.; et al. (2014). "Origin of igneous meteorites and differentiated asteroids". Asteroids. ACM: 483. Bibcode:2014acm..conf..483S.

mit.edu

dspace.mit.edu

Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.

nasa.gov

ssd.jpl.nasa.gov

"spec. type (Tholen) is defined". JPL Solar System Dynamics. JPL Small-Body Database Search Engine. JPL. Retrieved 26 Dec 2021.
"spec. type (Tholen) = M". JPL Solar System Dynamics. JPL Small-Body Database Search Engine. JPL. Retrieved 26 Dec 2021.
"spec. type (Tholen) = X AND albedo >= 0.1 AND albedo <= 0.3". JPL Solar System Dynamics. JPL Small-Body Database Search Engine. JPL. Retrieved 26 Dec 2021.

nih.gov

pubmed.ncbi.nlm.nih.gov

Elkins-Tanton, L. T.; et al. (2020). "Observations, meteorites, and models: A preflight assessment of the composition and formation of (16) Psyche". Journal of Geophysical Research: Planets. 125 (3): 23. doi:10.1029/2019JE006296. PMC 7375145. PMID 32714727. S2CID 214018872.
Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.
Coradini, A.; et al. (2011). "The surface composition and temperature of asteroid 21 Lutetia as observed by Rosetta/VIRTIS". Science. 334 (492): 492–494. doi:10.1126/science.1204062. PMID 22034430. S2CID 19439721.
Margot, J.L.; Brown, M.E. (2003). "A low-density M-type asteroid in the main belt". Science. 300 (5627): 1939–1942. doi:10.1126/science.1085844. PMID 12817147. S2CID 5479442.

ncbi.nlm.nih.gov

Elkins-Tanton, L. T.; et al. (2020). "Observations, meteorites, and models: A preflight assessment of the composition and formation of (16) Psyche". Journal of Geophysical Research: Planets. 125 (3): 23. doi:10.1029/2019JE006296. PMC 7375145. PMID 32714727. S2CID 214018872.

semanticscholar.org

api.semanticscholar.org

Bus, S.J.; Binzel, R.P. (2002). "Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy". Icarus. 158 (1): 146–177. Bibcode:2002Icar..158..146B. doi:10.1006/icar.2002.6856. S2CID 4880578.
Pitjeva, E.V.; Pitjev, N.P. (2018). "Masses of the main asteroid belt and the Kuiper belt from the motions of planets and spacecraft". Earth and Planetary Astrophysics. 44 (8–9): 554–566. arXiv:1811.05191v1. doi:10.1134/S1063773718090050. S2CID 255197841.
Elkins-Tanton, L. T.; et al. (2020). "Observations, meteorites, and models: A preflight assessment of the composition and formation of (16) Psyche". Journal of Geophysical Research: Planets. 125 (3): 23. doi:10.1029/2019JE006296. PMC 7375145. PMID 32714727. S2CID 214018872.
Shepard, M.K.; et al. (2021). "Asteroid 16 Psyche: Shape, features, and global map". The Planetary Science Journal. 2 (4): 16. arXiv:2110.03635. doi:10.3847/PSJ/abfdba. S2CID 235918955.
Sierks, H.; et al. (2011). "Images of asteroid 21 Lutetia: A remnant planetesimal from the early Solar system" (PDF). Science. 334 (6055): 487–490. Bibcode:2011Sci...334..487S. doi:10.1126/science.1207325. hdl:1721.1/110553. PMID 22034428. S2CID 17580478.
Vernazza, P.; et al. (2021). "VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis". Astronomy and Astrophysics. 654 (A56): 48. doi:10.1051/0004-6361/202141781. hdl:10261/263281. S2CID 239104699.
Carry, B. (2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.
Marchis, F.; Jorda, L.; Vernazza, P.; Brož, M.; Hanuš, J.; Ferrais, M.; et al. (September 2021). "(216) Kleopatra, a low density, critically rotating, M-type asteroid". Astronomy & Astrophysics. 653: A57. arXiv:2108.07207. doi:10.1051/0004-6361/202140874. S2CID 237091036. A57. Retrieved 13 October 2021.
Descamps, P.; Marchis, F.; Pollock, J.; Berthier, J.; Vachier, F.; Birlan, M.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. S2CID 118437111.
Johnson, B.C.; Sori, M.M.; Evans, A.J. (2020). "Ferrovolcanism of metal worlds and the origin of pallasites". Nature Astronomy. 4: 41–44. arXiv:1909.07451. doi:10.1038/s41550-019-0885-x. S2CID 202583406.
Coradini, A.; et al. (2011). "The surface composition and temperature of asteroid 21 Lutetia as observed by Rosetta/VIRTIS". Science. 334 (492): 492–494. doi:10.1126/science.1204062. PMID 22034430. S2CID 19439721.
Margot, J.L.; Brown, M.E. (2003). "A low-density M-type asteroid in the main belt". Science. 300 (5627): 1939–1942. doi:10.1126/science.1085844. PMID 12817147. S2CID 5479442.
Descamps, P.; et al. (2011). "Triplicity and physical characteristics of asteroid (216) Kleopatra". Icarus. 245 (2): 64–69. arXiv:1011.5263. doi:10.1016/j.icarus.2010.11.016. S2CID 119286272.

semanticscholar.org

Bus, S.J.; Binzel, R.P. (2002). "Phase II of the Small Main-belt Asteroid Spectroscopy Survey: A feature-based taxonomy". Icarus. 158 (1): 146–177. Bibcode:2002Icar..158..146B. doi:10.1006/icar.2002.6856. S2CID 4880578.