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2696 Magion

From Wikipedia, the free encyclopedia
Main-belt asteroid

2696 Magion
Discovery[1]
Discovered byL. Brožek
Discovery siteKleť Obs.
Discovery date16 April 1980
Designations
(2696) Magion
Named after
Magion 1[2]
(Czechoslovaksatellite)
1980 HB · 1951 SK
1953 GC · 1978 TN7
main-belt[1][3] · (inner)
background[4][5] · Phocaea[6]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc66.41yr (24,255 d)
Aphelion2.7287AU
Perihelion2.1712 AU
2.4499 AU
Eccentricity0.1138
3.83 yr (1,401 d)
35.557°
0° 15m 25.2s / day
Inclination25.350°
186.23°
283.31°
Physical characteristics
10.06 km(calculated)[6]
20.18±1.0 km[7]
20.83±5.49 km[8]
21.388±0.121 km[9]
22.74±0.53 km[10]
23.824±8.215 km[11]
25.418±0.186 km[12]
480±h[13][a]
0.0345±0.0036[12]
0.038±0.004[9]
0.04±0.03[8]
0.0421±0.0397[11]
0.054±0.003[10]
0.0687±0.008[7]
0.23(assumed)[6]
X[14] · S(assumed)[6]
12.00[7][10][12]
12.20[3][6][11]
12.39[8]
12.48±0.02[14]

2696 Magion, provisional designation1980 HB, is a dark backgroundasteroid and aslow rotator from the inner regions of theasteroid belt, approximately 21 kilometers (13 miles) in diameter. It was discovered on 16 April 1980, by Slovak astronomerLadislav Brožek at theKleť Observatory in former Czechoslovakia.[1] TheX-type asteroid has an ambiguousrotation period of 480 hours and is possibly atumbler.[6] It was named for the first Czechoslovaksatellite,Magion 1, launched in 1978.[2]

Orbit and classification

[edit]

Magion is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4][5] Based on osculating Keplerianorbital elements, the asteroid has also been considered a member of thePhocaea family (701),[6] a large family with two thousand members, named after25 Phocaea.

It orbits the Sun in theinner asteroid belt at a distance of 2.2–2.7 AU once every 3 years and 10 months (1,401 days;semi-major axis of 2.45 AU). Its orbit has aneccentricity of 0.11 and aninclination of 25° with respect to theecliptic.[3] The body'sobservation arc begins with its first observation as1951 SK atGoethe Link Observatory in September 1951, more than 28 years prior to its official discovery observation at Kleť.[1]

Physical characteristics

[edit]

Magion has been characterized as anX-type asteroid byPan-STARRS large-scale survey.[14] It is also an assumedS-type asteroid based on its family classification.[6]

Rotation period and slow rotator

[edit]

In May 2007, a rotationallightcurve ofMagion was obtained fromphotometric observations by astronomersAdrián Galád,Leonard Kornoš andŠtefan Gajdoš atModra Observatory in Slovakia. Lightcurve analysis gave an exceptionally long but ambiguousrotation period of480±6 hours with a brightness amplitude of 0.31magnitude (U=2).[13] Alternative periods are 474 and 360 hours, respectively.[a] Due to its long period, thisslow rotator ranks among to theTop 100 of its kind. It may also be atumbler, yet no strong evidence has been found (T0).[6][b]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Magion measures between 20.18 and 25.418 kilometers in diameter and its surface has analbedo between 0.0345 and 0.0687.[7][8][9][10][11][12]

TheCollaborative Asteroid Lightcurve Link assumes a high albedo of 0.23 – derived from 25 Phocaea, the parent body of the Phocaea family – and consequently calculates a much smaller diameter of 10.06 kilometers based on anabsolute magnitude of 12.2.[6]

Naming

[edit]

Thisminor planet was named after "Magion 1", the first Czechoslovakartificial satellite, launched withInterkosmos 18 mission on 24 October 1978. The satellite studied the interactions betweenEarth's magnetosphere and itsionosphere, and it examined the special structure ofextremely low frequency waves.[2] The official naming citation was published by theMinor Planet Center on 28 January 1983 (M.P.C. 7620).[15]

Notes

[edit]
  1. ^abLightcurve plot of (2696) Magion taken by Galad and Pravec at Modra in June 2007, with an ambiguous rotation period474 (or 350) hours. Quality code of 2. Summary figures at theLCDB.
  2. ^PAR = 0. See (2696) Magion at theLCDB. Definition by the LCDB for PAR = 0:The tumbling damping time scale is long enough that tumbling might be expected, but observations are not sufficient to substantiate either tumbling or not tumbling (fromNOTES (single letter flag(s)).

References

[edit]
  1. ^abcd"2696 Magion (1980 HB)".Minor Planet Center. Retrieved12 April 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(2696) Magion".Dictionary of Minor Planet Names – (2696) Magion. Springer Berlin Heidelberg. p. 220.doi:10.1007/978-3-540-29925-7_2697.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 2696 Magion (1980 HB)" (2018-02-25 last obs.).Jet Propulsion Laboratory. Retrieved12 April 2018.
  4. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved12 April 2018.
  5. ^ab"Asteroid 2696 Magion – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcdefghij"LCDB Data for (2696) Magion". Asteroid Lightcurve Database (LCDB). Retrieved12 April 2018.
  7. ^abcdTedesco, 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. Retrieved22 October 2019.
  8. ^abcdNugent, 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.
  9. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved12 April 2018.
  10. ^abcdUsui, 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)
  11. ^abcdMasiero, 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.
  12. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 35447010.
  13. ^abGalad, Adrian; Kornos, Leonard; Gajdos, Stefan (January 2009)."Lightcurves of Eight Selected Asterois from Modra".The Minor Planet Bulletin.36 (1):13–15.Bibcode:2009MPBu...36...13G.ISSN 1052-8091. Retrieved12 April 2018.
  14. ^abcVeres, 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.
  15. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved12 April 2018.

External links

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