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881 Athene

From Wikipedia, the free encyclopedia
Stony background asteroid

881 Athene
Modelled shape ofAthene from itslightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 July 1917
Designations
(881) Athene
Pronunciation/əˈθn/[2]
Named after
GoddessAthena
(Greek mythology)[3]
A917 OD · 1917 CL
AdjectivesAthenian/əˈθniən/
Orbital characteristics[4]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc102.53yr (37,449 d)
Aphelion3.1510AU
Perihelion2.0764 AU
2.6137 AU
Eccentricity0.2056
4.23 yr (1,543 d)
121.30°
0° 13m 59.52s / day
Inclination14.191°
277.03°
41.313°
Physical characteristics
  • (123.0°, −58.0°) (λ11)[6]
  • (337.0°, −47.0°) (λ22)[6]
  • 0.237±0.039[8]
  • 0.237±0.012[7]
11.8[1][4]

881 Athene (prov. designation:A917 ODor1917 CL) is a stonybackground asteroid from the central region of theasteroid belt. It was discovered on 22 July 1917, by astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory in southwest Germany.[1] The likely elongatedS/L-type asteroid has arotation period of 13.9 hours and measures approximately 12 kilometers (7.5 miles) in diameter. It was named afterAthena, the goddess of wisdom inGreek mythology.[3]According to Astrophysicist Rayme Traub at JHU APL NASA, Europa Clipper will make a pass by Athene in 2027 after passing Earth on its way to Jupiter. Europa Clipper will test its sensors on Athene in preparation for Europa in 2030.

Orbit and classification

[edit]

Located in or near the orbital region of theEunomia family,[11]Athene is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[5][6] It orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.2 AU once every 4 years and 3 months (1,543 days;semi-major axis of 2.61 AU). Its orbit has aneccentricity of 0.21 and aninclination of 14° with respect to theecliptic.[4] The body'sobservation arc begins atUccle Observatory on 8 August 1934, almost 17 years after its official discovery observation at Heidelberg on 22 July 1917.[1]

Naming

[edit]

Thisminor planet was named afterAthena or "Pallas Athene", the goddess of wisdom inGreek mythology, also known asMinerva inRoman mythology. Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 86). Asteroids93 Minerva and2 Pallas are both named after the goddess as well.[3]

Physical characteristics

[edit]

In the Tholen-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2),Athene is a common, stonyS-type asteroid, while in theSDSS-based taxonomy, it is anL-type asteroid.[10] In the SMASS-like taxonomic variant of the S3OS2,Athene is an Sl-subtype that transitions between the S-and L-type.[6][9]

Rotation period

[edit]

In August 2006, a rotationallightcurve ofAthene was obtained fromphotometric observations by Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station (A12), Italy, and by Jean-Gabriel Bosch at the Collonges Observatory (178), France. Lightcurve analysis gave arotation period of13.895±0.003 hours with a high brightness variation of0.53±0.01magnitude, indicative of a non-spherical, elongated shape (U=3−). In September 2010, French amateur astronomerRené Roy measured a similar period of13.881±0.001 hours and an amplitude of0.39±0.02 (U=2+).[12][11]

Poles

[edit]

Two lightcurves, published in 2016, using modeled photometric data from the Lowell Photometric Database (LPD) and other sources, gave a concurring sidereal period of13.89449±0.00001 and13.8943±0.0005 hours, respectively. Each modeled lightcurve also determined twospin axes of (123.0°, −58.0°) and (337.0°, −47.0°), as well as (115.0°, −77.0°) and (338.0°, −43.0°) inecliptic coordinates (λ, β).[6][13][14]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Athene measures (12.04±0.28) and (12.153±0.101) kilometers in diameter and its surface has analbedo of (0.237±0.012) and (0.237±0.039), respectively.[7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard Eunomian albedo of 0.21 and calculates a diameter of 12.66 kilometers based on anabsolute magnitude of 11.8.[11] Alternativemean diameter measurements published by the WISE team include (12.152±2.176 km), (12.369±0.285 km) and (12.671±0.077 km) with corresponding albedos of (0.278±0.128), (0.241±0.044) and (0.2111±0.0234).[6][11]

References

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  1. ^abcde"881 Athene (A917 OD)".Minor Planet Center. Retrieved27 February 2020.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^abcSchmadel, Lutz D. (2007). "(881) Athene".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 79.doi:10.1007/978-3-540-29925-7_882.ISBN 978-3-540-00238-3.
  4. ^abcd"JPL Small-Body Database Browser: 881 Athene (A917 OD)" (2020-02-01 last obs.).Jet Propulsion Laboratory. Retrieved27 February 2020.
  5. ^ab"Asteroid 881 Athene – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved27 February 2020.
  6. ^abcdefg"Asteroid 881 Athene".Small Bodies Data Ferret. Retrieved27 February 2020.
  7. ^abcUsui, 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)
  8. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.
  9. ^abcLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved27 February 2020.
  10. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved27 February 2020.(PDS data set)
  11. ^abcd"LCDB Data for (881) Athene". Asteroid Lightcurve Database (LCDB). Retrieved27 February 2020.
  12. ^Behrend, Raoul."Asteroids and comets rotation curves – (881) Athene".Geneva Observatory. Retrieved27 February 2020.
  13. ^Ďurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: A48.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.ISSN 0004-6361.
  14. ^Hanuš, J.; Ďurech, 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: A108.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.ISSN 0004-6361.

External links

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