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Maja (minor planet designation : 66 Maja ) is a carbonaceous background asteroid from the central regions of the asteroid belt , approximately 71 kilometers in diameter. It was discovered on 9 April 1861, by American astronomer Horace Tuttle at the Harvard College Observatory in Cambridge, Massachusetts, United States.[21] The asteroid was named after Maia from Greek mythology.[3]
Orbit and classification [ edit ]
Maja is a non-family asteroid from the main belt's background population .[5] It orbits the Sun in the central asteroid belt at a distance of 2.2–3.1 AU once every 4 years and 4 months (1,571 days; semi-major axis of 2.65 AU ). Its orbit has an eccentricity of 0.17 and an inclination of 3° with respect to the ecliptic .[1] The body's observation arc begins at the Harvard Observatory, one night after its official discovery observation.[21]
Physical characteristics [ edit ]
In the Tholen classification , Maja is a carbonaceous C-type asteroid ,[1] while in the SMASS classification it is a "hydrated" carbonaceous subtype (Ch ).[1]
Rotation period and spin axes [ edit ]
Several rotational lightcurves of Maja have been obtained from photometric observations since 1988.[13] [14] [15] [17] [18] Analysis of the best-rated lightcurve by French amateur astronomers Maurice Audejean and Jérôme Caron from February 2011 gave a rotation period of 9.73509 hours with a brightness amplitude of 0.25 magnitude (U=3 ).[4] [15]
In 2016, a modeled lightcurve was derived from various photometric database sources, giving a concurring sidereal period of 9.73570 hours and two spin axes of (49.0°, −70.0°) and (225.0°, −68.0°) in ecliptic coordinates .[16]
Diameter and albedo [ edit ]
According to the surveys carried out by the Infrared Astronomical Satellite IRAS , the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Maja measures between 62.87 and 82.28 kilometers in diameter and its surface has an albedo between 0.03 and 0.0759.[6] [7] [8] [9] [10] [11]
The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0618 and a diameter of 71.82 kilometers based on an absolute magnitude of 9.36.[4] [9]
This minor planet was named by Harvard 's former president, J. Quincy, after Maia , one of the Seven Sisters of the Pleiades in Greek mythology . She is the mother of Hermes (Mercury) and the daughter of Atlas and Pleione . The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 10 ).[3]
The asteroids 130 Elektra , 233 Asterope and 1051 Merope were also named after the mythological Seven Sisters. In 1861, the director of the discovering observatory, George Phillips Bond , raised a minor concern since these names had already been applied to some of the brightest stars of the Pleiades in the constellation of Taurus: Maia , Electra , Asterope and Merope .[3]
Spacecraft visits [ edit ]
At present, Maja has not been visited by any spacecraft. As of 1988, mission planning for the Cassini–Huygens spacecraft included a flyby of Maja while leaving the inner solar system in March 1997, however due to delays, the launch of Cassini-Huygens was moved from April 1996 to October 1997, thus negating the option to pass near Maja . Cassini-Huygens passed by asteroid 2685 Masursky on 23 January 2000 instead.[22]
References [ edit ]
^ 'Maia' in Noah Webster (1884) A Practical Dictionary of the English Language
^ a b c d Schmadel, Lutz D. (2007). "(66 ) Maja". Dictionary of Minor Planet Names – (66 ) Maja . Springer Berlin Heidelberg . pp. 21–22. doi :10.1007/978-3-540-29925-7_67 . ISBN 978-3-540-00238-3 .
^ a b c d e "LCDB Data for (66 ) Maja" . Asteroid Lightcurve Database (LCDB). Retrieved 11 January 2018 .
^ a b "Asteroid 66 Maja" . Small Bodies Data Ferret . Retrieved 24 October 2019 .
^ a b c d e Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos" . The Astrophysical Journal . 814 (2 ): 13. arXiv :1509.02522 . Bibcode :2015ApJ...814..117N . doi :10.1088/0004-637X/814/2/117 . S2CID 9341381 . Retrieved 11 January 2018 .
^ a b c d Masiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017). "NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos" . The Astronomical Journal . 154 (4 ): 10. arXiv :1708.09504 . Bibcode :2017AJ....154..168M . doi :10.3847/1538-3881/aa89ec .
^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey" . Publications of the Astronomical Society of Japan . 63 (5 ): 1117–1138. Bibcode :2011PASJ...63.1117U . doi :10.1093/pasj/63.5.1117 . (online , AcuA catalog p. 153 )
^ a b c d e Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0" . NASA Planetary Data System . 12 : IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode :2004PDSS...12.....T . Retrieved 22 October 2019 .
^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids" . The Astrophysical Journal Letters . 759 (1 ): 5. arXiv :1209.5794 . Bibcode :2012ApJ...759L...8M . doi :10.1088/2041-8205/759/1/L8 . S2CID 46350317 . Retrieved 11 January 2018 .
^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos" . The Astronomical Journal . 152 (3 ): 12. arXiv :1606.08923 . Bibcode :2016AJ....152...63N . doi :10.3847/0004-6256/152/3/63 .
^ Krasinsky, G. A.; Pitjeva, E. V.; Vasilyev, M. V.; Yagudina, E. I. (2002). "Hidden Mass in the Asteroid Belt" . Icarus . 158 (1 ): 98. Bibcode :2002Icar..158...98K . doi :10.1006/icar.2002.6837 .
^ a b di Martino, M.; Ferreri, W.; Fulchignoni, M.; de Angelis, G.; Barucci, M. A. (October 1990). "66 Maja and 951 Gaspra - Possible flyby targets for Cassini and Galileo missions" . Icarus . 87 (2 ): 372–376. Bibcode :1990Icar...87..372D . doi :10.1016/0019-1035(90 )90140-5 . ISSN 0019-1035 . Retrieved 11 January 2018 .
^ a b Barucci, M. A.; Fulchignoni, M.; di Martino, M. (June 1989). "Observations of Asteroids 66 Maja and 951 Gaspra, Possible Flyby Targets for "Cassini" and "Galileo" Missions" . Bulletin of the American Astronomical Society . 21 : 963. Bibcode :1989BAAS...21..963B . Retrieved 11 January 2018 .
^ a b c d Behrend, Raoul. "Asteroids and comets rotation curves – (66 ) Maja" . Geneva Observatory. Retrieved 11 January 2018 .
^ a b Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". Astronomy and Astrophysics . 586 : 24. arXiv :1510.07422 . Bibcode :2016A&A...586A.108H . doi :10.1051/0004-6361/201527441 . S2CID 119112278 .
^ a b Ditteon, Richard; Hawkins, Scot (September 2007). "Asteroid Lightcurve Analysis at the Oakley Observatory - October-November 2006" . The Minor Planet Bulletin . 34 (3 ): 59–64. Bibcode :2007MPBu...34...59D . ISSN 1052-8091 . Retrieved 11 January 2018 .
^ a b Riccioli, D.; Blanco, C.; Cigna, M. (June 2001). "Rotational periods of asteroids II" . Planetary and Space Science . 49 (7 ): 657–671. Bibcode :2001P&SS...49..657R . doi :10.1016/S0032-0633(01 )00014-9 . Retrieved 11 January 2018 .
^ a b Warner, Brian D. (December 2007). "Initial Results of a Dedicated H-G Project" . The Minor Planet Bulletin . 34 (4 ): 113–119. Bibcode :2007MPBu...34..113W . ISSN 1052-8091 . Retrieved 11 January 2018 .
^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results" . Icarus . 261 : 34–47. arXiv :1506.00762 . Bibcode :2015Icar..261...34V . doi :10.1016/j.icarus.2015.08.007 . S2CID 53493339 . Retrieved 11 January 2018 .
^ a b "66 Maja" . Minor Planet Center . Retrieved 11 January 2018 .
^ Outward to the Beginning: the CRAF and Cassini Missions of the Mariner Mark 2 Program ; NASA Contractor Report CR-183133, 1 June 1988
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=66_Maja&oldid=1230786896 "
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