3200 Phaethon (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "3200 Phaethon" in English language version.

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12harvard.edu

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10arxiv.org

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10doi.org

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7semanticscholar.org

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7nasa.gov

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4web.archive.org

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2iop.org

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2spacedys.com

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1archive.today

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1oed.com

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1minorplanetcenter.net

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1hal-astro-lab.com

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1ucla.edu

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1nationalgeographic.org

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1worldcat.org

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1skymania.com

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1earthsky.org

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1cnet.com

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1ucf.edu

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1space.com

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1jaxa.jp

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1cam.ac.uk

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archive.today

In 2014, JPL 374 (solution date 2014-Sep-12) showed a 2017 Earth approach distance with a precision of ±80 km. Math: (MAX−MIN) * AU / 2

arxiv.org

Kartashova, A.; Husarik, M.; Ivanova, O.; Kokhirova, G.; Bakanas, E.; Sokolov, I.; Khamroev, U. Kh.; Ibragimov, A. A. (June 5, 2019), "Photometric observations of the asteroid 3200 Phaethon using small and middle telescopes", Contributions of the Astronomical Observatory Skalnate Pleso, 49 (2): 367, arXiv:1906.01064, Bibcode:2019CoSka..49..367K
Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". In Michel, P.; et al. (eds.). Asteroids IV (PDF). University of Arizona. pp. 221–241. arXiv:1502.02361. Bibcode:2015aste.book..221J. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 9780816532131. S2CID 119209764. Retrieved January 30, 2020.
Cukier, W. Z.; Szalay, J. R. (June 1, 2023). "Formation, Structure, and Detectability of the Geminids Meteoroid Stream". The Planetary Science Journal. 4 (6): 109. arXiv:2306.11151. Bibcode:2023PSJ.....4..109C. doi:10.3847/psj/acd538. ISSN 2632-3338.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". The Astronomical Journal. 140 (5): 1519. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528.
Jewitt, David; Li, Jing; Agarwal, Jessica (2013). "The Dust Tail of Asteroid (3200) Phaethon". The Astrophysical Journal Letters. 771 (2). L36. arXiv:1306.3741. Bibcode:2013ApJ...771L..36J. doi:10.1088/2041-8205/771/2/L36. S2CID 37387069.
Li, Jing; Jewitt, David (2013). "Recurrent Perihelion Activity in (3200) Phaethon". Astronomical Journal. 145 (6): 154. arXiv:1304.1430. Bibcode:2013AJ....145..154L. doi:10.1088/0004-6256/145/6/154. S2CID 6242944. Retrieved January 22, 2022.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". Astronomical Journal. 140 (5): 1519–1527. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528. Retrieved January 22, 2022.
Golubeva, L. F.; Shestopalov, D. I.; Kvaratskhelia, O. I. (2020). "Polarimetric properties of asteroid 3200 Phaethon". arXiv:2001.00789 [astro-ph.EP].
Lisse, Carey; Steckloff, Jordan (2022). "Thermal alteration and differential sublimation can create Phaethon's "rock comet" activity and blue color". Icarus. 381: 114995. arXiv:2203.09876. Bibcode:2022Icar..38114995L. doi:10.1016/j.icarus.2022.114995. S2CID 247594726.
MacLennan, Eric; Granvik, Mikael (November 2, 2023). "Thermal decomposition as the activity driver of near-Earth asteroid (3200) Phaethon". Nature Astronomy. arXiv:2207.08968. doi:10.1038/s41550-023-02091-w.

cam.ac.uk

ast.cam.ac.uk

Shanklin, Jonathan (2009). "Comet Section: 2009 News". British Astronomical Association. Retrieved September 20, 2009.

cnet.com

Eric Mack (October 23, 2018). "A look at 3200 Phaethon: A big, bizarre, blue asteroid we plan to visit". CNET. Retrieved April 6, 2019.

doi.org

Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". In Michel, P.; et al. (eds.). Asteroids IV (PDF). University of Arizona. pp. 221–241. arXiv:1502.02361. Bibcode:2015aste.book..221J. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 9780816532131. S2CID 119209764. Retrieved January 30, 2020.
Devogèle, Maxime; MacLennan, Eric; Gustafsson, Annika; Moskovitz, Nicholas; Chatelain, Joey; Borisov, Galin; et al. (June 2020). "New Evidence for a Physical Link between Asteroids (155140) 2005 UD and (3200) Phaethon". The Planetary Science Journal. 1 (1): 15. Bibcode:2020PSJ.....1...15D. doi:10.3847/PSJ/ab8e45. 15.
Cukier, W. Z.; Szalay, J. R. (June 1, 2023). "Formation, Structure, and Detectability of the Geminids Meteoroid Stream". The Planetary Science Journal. 4 (6): 109. arXiv:2306.11151. Bibcode:2023PSJ.....4..109C. doi:10.3847/psj/acd538. ISSN 2632-3338.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". The Astronomical Journal. 140 (5): 1519. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528.
Jewitt, David; Li, Jing; Agarwal, Jessica (2013). "The Dust Tail of Asteroid (3200) Phaethon". The Astrophysical Journal Letters. 771 (2). L36. arXiv:1306.3741. Bibcode:2013ApJ...771L..36J. doi:10.1088/2041-8205/771/2/L36. S2CID 37387069.
Li, Jing; Jewitt, David (2013). "Recurrent Perihelion Activity in (3200) Phaethon". Astronomical Journal. 145 (6): 154. arXiv:1304.1430. Bibcode:2013AJ....145..154L. doi:10.1088/0004-6256/145/6/154. S2CID 6242944. Retrieved January 22, 2022.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". Astronomical Journal. 140 (5): 1519–1527. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528. Retrieved January 22, 2022.
Clark, Beth; Ziffer, Julie; Nesvorny, David (2010). "Spectroscopy of B-type asteroids: Subgroups and meteorite analogs". Journal of Geophysical Research. 115 (E6): E06005. Bibcode:2010JGRE..115.6005C. doi:10.1029/2009JE003478. S2CID 130052649.
Lisse, Carey; Steckloff, Jordan (2022). "Thermal alteration and differential sublimation can create Phaethon's "rock comet" activity and blue color". Icarus. 381: 114995. arXiv:2203.09876. Bibcode:2022Icar..38114995L. doi:10.1016/j.icarus.2022.114995. S2CID 247594726.
MacLennan, Eric; Granvik, Mikael (November 2, 2023). "Thermal decomposition as the activity driver of near-Earth asteroid (3200) Phaethon". Nature Astronomy. arXiv:2207.08968. doi:10.1038/s41550-023-02091-w.

earthsky.org

Eleanor Imster (November 1, 2018). "Rare blue asteroid sometimes behaves like a comet". EarthSky. Retrieved April 6, 2019.

hal-astro-lab.com

"(3200) Phaethon 2021 Oct 3". Hayamizu Astro Laboratory. October 3, 2021. Retrieved February 14, 2022.

harvard.edu

ui.adsabs.harvard.edu

Kartashova, A.; Husarik, M.; Ivanova, O.; Kokhirova, G.; Bakanas, E.; Sokolov, I.; Khamroev, U. Kh.; Ibragimov, A. A. (June 5, 2019), "Photometric observations of the asteroid 3200 Phaethon using small and middle telescopes", Contributions of the Astronomical Observatory Skalnate Pleso, 49 (2): 367, arXiv:1906.01064, Bibcode:2019CoSka..49..367K
Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". In Michel, P.; et al. (eds.). Asteroids IV (PDF). University of Arizona. pp. 221–241. arXiv:1502.02361. Bibcode:2015aste.book..221J. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 9780816532131. S2CID 119209764. Retrieved January 30, 2020.
Devogèle, Maxime; MacLennan, Eric; Gustafsson, Annika; Moskovitz, Nicholas; Chatelain, Joey; Borisov, Galin; et al. (June 2020). "New Evidence for a Physical Link between Asteroids (155140) 2005 UD and (3200) Phaethon". The Planetary Science Journal. 1 (1): 15. Bibcode:2020PSJ.....1...15D. doi:10.3847/PSJ/ab8e45. 15.
Cukier, W. Z.; Szalay, J. R. (June 1, 2023). "Formation, Structure, and Detectability of the Geminids Meteoroid Stream". The Planetary Science Journal. 4 (6): 109. arXiv:2306.11151. Bibcode:2023PSJ.....4..109C. doi:10.3847/psj/acd538. ISSN 2632-3338.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". The Astronomical Journal. 140 (5): 1519. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528.
Jewitt, David; Li, Jing; Agarwal, Jessica (2013). "The Dust Tail of Asteroid (3200) Phaethon". The Astrophysical Journal Letters. 771 (2). L36. arXiv:1306.3741. Bibcode:2013ApJ...771L..36J. doi:10.1088/2041-8205/771/2/L36. S2CID 37387069.
Li, Jing; Jewitt, David (2013). "Recurrent Perihelion Activity in (3200) Phaethon". Astronomical Journal. 145 (6): 154. arXiv:1304.1430. Bibcode:2013AJ....145..154L. doi:10.1088/0004-6256/145/6/154. S2CID 6242944. Retrieved January 22, 2022.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". Astronomical Journal. 140 (5): 1519–1527. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528. Retrieved January 22, 2022.
Clark, Beth; Ziffer, Julie; Nesvorny, David (2010). "Spectroscopy of B-type asteroids: Subgroups and meteorite analogs". Journal of Geophysical Research. 115 (E6): E06005. Bibcode:2010JGRE..115.6005C. doi:10.1029/2009JE003478. S2CID 130052649.
Lisse, Carey; Steckloff, Jordan (2022). "Thermal alteration and differential sublimation can create Phaethon's "rock comet" activity and blue color". Icarus. 381: 114995. arXiv:2203.09876. Bibcode:2022Icar..38114995L. doi:10.1016/j.icarus.2022.114995. S2CID 247594726.
Whipple, F. L. (October 25, 1983). Marsden, B. G. (ed.). "1983 TB and the Geminid Meteors". IAU Circular. 3881. 1. Bibcode:1983IAUC.3881....1W.
Battams, K.; Watson, A. (June 2009). "(3200) Phaethon". IAU Circular. 9054. 3. Bibcode:2009IAUC.9054....3B.

iop.org

iopscience.iop.org

Li, Jing; Jewitt, David (2013). "Recurrent Perihelion Activity in (3200) Phaethon". Astronomical Journal. 145 (6): 154. arXiv:1304.1430. Bibcode:2013AJ....145..154L. doi:10.1088/0004-6256/145/6/154. S2CID 6242944. Retrieved January 22, 2022.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". Astronomical Journal. 140 (5): 1519–1527. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528. Retrieved January 22, 2022.

jaxa.jp

Kuninaka, Hitoshi (May 19, 2020). "宇宙科学ミッション打上げ計画について" (PDF) (in Japanese). JAXA. Retrieved September 28, 2020.

minorplanetcenter.net

"(3200) Phaethon Orbit". Minor Planet Center. Retrieved June 5, 2019.

nasa.gov

ssd.jpl.nasa.gov

"JPL Small-Body Database: 3200 Phaethon (1983 TB)". JPL Small-Body Database. Jet Propulsion Laboratory. Archived from the original on June 5, 2019. Retrieved June 5, 2019.
JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive.)
"JPL Small-Body Database Search Engine — Constraints: asteroids and q < 0.141 (au)". JPL Small-Body Database. Jet Propulsion Laboratory. Retrieved September 5, 2011. Take notice of the orbit condition number (the lower the number, the lower the orbit's uncertainty).

jpl.nasa.gov

Agle, D. C.; Brown, Dwayne; Farukhi, Suraiya (December 22, 2017). "Arecibo Radar Returns with Asteroid Phaethon Images". NASA. Retrieved January 8, 2018.

echo.jpl.nasa.gov

Benner, Lance A. M. (2017). "Goldstone Radar Observations Planning: Asteroid 3200 Phaethon". NASA/JPL Asteroid Radar Research. Retrieved November 26, 2017.

science.nasa.gov

Phillips, Tony (December 3, 2007). "Asteroid Shower". Science@NASA. NASA. Retrieved April 4, 2017.

cneos.jpl.nasa.gov

"NEO Groups". Near Earth Object Program. NASA. Archived from the original on November 2, 2016.

nationalgeographic.org

voices.nationalgeographic.org

Jaggard, Victoria (October 12, 2010). "Exploding Clays Drive Geminids Sky Show?". National Geographic. Archived from the original on August 11, 2017. Retrieved August 10, 2017.

oed.com

"phaeton". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)

semanticscholar.org

api.semanticscholar.org

Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". In Michel, P.; et al. (eds.). Asteroids IV (PDF). University of Arizona. pp. 221–241. arXiv:1502.02361. Bibcode:2015aste.book..221J. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 9780816532131. S2CID 119209764. Retrieved January 30, 2020.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". The Astronomical Journal. 140 (5): 1519. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528.
Jewitt, David; Li, Jing; Agarwal, Jessica (2013). "The Dust Tail of Asteroid (3200) Phaethon". The Astrophysical Journal Letters. 771 (2). L36. arXiv:1306.3741. Bibcode:2013ApJ...771L..36J. doi:10.1088/2041-8205/771/2/L36. S2CID 37387069.
Li, Jing; Jewitt, David (2013). "Recurrent Perihelion Activity in (3200) Phaethon". Astronomical Journal. 145 (6): 154. arXiv:1304.1430. Bibcode:2013AJ....145..154L. doi:10.1088/0004-6256/145/6/154. S2CID 6242944. Retrieved January 22, 2022.
Jewitt, David; Li, Jing (2010). "Activity in Geminid Parent (3200) Phaethon". Astronomical Journal. 140 (5): 1519–1527. arXiv:1009.2710. Bibcode:2010AJ....140.1519J. doi:10.1088/0004-6256/140/5/1519. S2CID 6446528. Retrieved January 22, 2022.
Clark, Beth; Ziffer, Julie; Nesvorny, David (2010). "Spectroscopy of B-type asteroids: Subgroups and meteorite analogs". Journal of Geophysical Research. 115 (E6): E06005. Bibcode:2010JGRE..115.6005C. doi:10.1029/2009JE003478. S2CID 130052649.
Lisse, Carey; Steckloff, Jordan (2022). "Thermal alteration and differential sublimation can create Phaethon's "rock comet" activity and blue color". Icarus. 381: 114995. arXiv:2203.09876. Bibcode:2022Icar..38114995L. doi:10.1016/j.icarus.2022.114995. S2CID 247594726.

skymania.com

Sutherland, Paul (September 10, 2013). "Why an asteroid is crumbling into meteor dust". Skymania.com. Archived from the original on February 22, 2015. Retrieved September 10, 2013.

space.com

How the bluest asteroid in the solar system got its color Tereza Pultarova, Space.com. June 16th, 2022

spacedys.com

newton.spacedys.com

"(3200) Phaethon: Ephemerides for December 2017". NEODyS-2. University of Pisa Department of Mathematics. Retrieved November 26, 2017.
"(3200) Phaethon: Close Approaches". NEODyS-2. University of Pisa Department of Mathematics. Retrieved May 18, 2009.

ucf.edu

stars.library.ucf.edu

Clark, Beth; Ziffer, Julie; Nesvorny, David (2010). "Spectroscopy of B-type asteroids: Subgroups and meteorite analogs". Journal of Geophysical Research. 115 (E6): E06005. Bibcode:2010JGRE..115.6005C. doi:10.1029/2009JE003478. S2CID 130052649.

ucla.edu

www2.ess.ucla.edu

Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". In Michel, P.; et al. (eds.). Asteroids IV (PDF). University of Arizona. pp. 221–241. arXiv:1502.02361. Bibcode:2015aste.book..221J. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 9780816532131. S2CID 119209764. Retrieved January 30, 2020.

web.archive.org

"JPL Small-Body Database: 3200 Phaethon (1983 TB)". JPL Small-Body Database. Jet Propulsion Laboratory. Archived from the original on June 5, 2019. Retrieved June 5, 2019.
Jaggard, Victoria (October 12, 2010). "Exploding Clays Drive Geminids Sky Show?". National Geographic. Archived from the original on August 11, 2017. Retrieved August 10, 2017.
"NEO Groups". Near Earth Object Program. NASA. Archived from the original on November 2, 2016.
Sutherland, Paul (September 10, 2013). "Why an asteroid is crumbling into meteor dust". Skymania.com. Archived from the original on February 22, 2015. Retrieved September 10, 2013.

worldcat.org

Cukier, W. Z.; Szalay, J. R. (June 1, 2023). "Formation, Structure, and Detectability of the Geminids Meteoroid Stream". The Planetary Science Journal. 4 (6): 109. arXiv:2306.11151. Bibcode:2023PSJ.....4..109C. doi:10.3847/psj/acd538. ISSN 2632-3338.