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F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
730 Athanasia (prov. designation : A912 GG or 1912 OK ) is a background asteroid from the inner regions of the asteroid belt , approximately 4.5 kilometers (2.8 miles) in diameter. It was discovered by Austrian astronomer Johann Palisa at the Vienna Observatory on 10 April 1912.[1] The presumed stony S-type asteroid has a rotation period of 5.7 hours and is likely very elongated in shape. It was named Athanasia , the Greek word for "immortality ".[3]
Orbit and classification [ edit ]
Located in the region of the Flora family (402 ),[10] a giant asteroid family and the largest family of stony asteroids in the main-belt, Athanasia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements .[5] [6] [7] It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,228 days; semi-major axis of 2.24 AU ). Its orbit has an eccentricity of 0.18 and an inclination of 4° with respect to the ecliptic .[4] The body's observation arc begins at Vienna Observatory on 15 April 1912, or five nights after its official discovery observation.[1]
This minor planet was named by friends of the discoverer after the Greek word for immortality , "athanasia". Any reference to a person or occurrence is unknown. The naming was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 73 ).[3]
Physical characteristics [ edit ]
Athanasia is an assumed, stony S-type asteroid .[10]
Rotation period [ edit ]
In February 2016, a rotational lightcurve of Athanasia was obtained from photometric observations by Frederick Pilcher at the Organ Mesa Observatory (G50 ) in New Mexico, United States. Analysis gave a classically shaped, well-defined bimodal lightcurve with a rotation period of 5.7348± 0.0001 hours and a very high brightness variation of 0.63± 0.04 magnitude , indicative of a highly elongated shape (U=3 ).[9] [a] In May 2013, Pilcher already observed the object and reported a ambiguous period of 5.7345or 8.6016 hours with an amplitude of 0.14 magnitude (U=2+ ).[11] [b]
Diameter and albedo [ edit ]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , Athanasia measures ( 4.497± 0.734 ) kilometers in diameter and its surface has a high albedo of ( 0.289± 0.123 ).[8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a Florian asteroid of 0.24 and calculates a diameter of 4.94 kilometers based on an absolute magnitude of 13.7.[10]
^ a b Lightcurve-plot of (730) Athanasia , by Frederick Pilcher at the Organ Mesa Observatory (2016). Rotation period of 5.7348 hours with a brightness amplitude of 0.63 mag. Quality code is 3. Summary figures at the LCDB and ALSC websites.
^ Lightcurve-plot of (730) Athanasia , by Frederick Pilcher at the Organ Mesa Observatory (2013). Rotation period of 5.7345 hours with a brightness amplitude of 0.14 mag. Quality code is 2+. Summary figures at the LCDB and ALSC websites.
References [ edit ]
^ 'Athanasius' in Noah Webster (1884) A Practical Dictionary of the English Language
^ a b c Schmadel, Lutz D. (2007). "(730) Athanasia". Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 70. doi :10.1007/978-3-540-29925-7_731 . ISBN 978-3-540-00238-3 .
^ a b c d e f "JPL Small-Body Database Browser: 730 Athanasia (A912 GG)" (2020-04-28 last obs.). Jet Propulsion Laboratory . Retrieved 10 June 2020 .
^ a b "Asteroid 730 Athanasia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved 10 June 2020 .
^ a b "Asteroid 730 Athanasia" . Small Bodies Data Ferret . Retrieved 10 June 2020 .
^ a b Zappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997). "Asteroid Dynamical Families" . NASA Planetary Data System : EAR-A-5-DDR-FAMILY-V4.1. Retrieved 10 June 2020 . } (PDS main page )
^ 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 .
^ a b Pilcher, Frederick (July 2016). "Rotation Period Determinations for 123 Brunhild, 314 Rosalia 346 Hermentaria, 633 Zelima, and 730 Athanasia" (PDF) . Minor Planet Bulletin . 43 (3 ): 222–224. Bibcode :2016MPBu...43..222P . ISSN 1052-8091 . Archived from the original (PDF) on 27 July 2021. Retrieved 10 June 2020 .
^ a b c d "LCDB Data for (730) Athanasia" . Asteroid Lightcurve Database (LCDB). Retrieved 10 June 2020 .
^ Pilcher, Frederick (October 2013). "Rotation Period Determination for 730 Athanasia" (PDF) . Minor Planet Bulletin . 40 (4 ): 194–195. Bibcode :2013MPBu...40..194P . ISSN 1052-8091 . Archived from the original (PDF) on 24 February 2020. Retrieved 10 June 2020 .
External links [ edit ]
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=730_Athanasia&oldid=1191340960 "
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