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1830 Pogson

From Wikipedia, the free encyclopedia
Asteroid

1830 Pogson
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date17 April 1968
Designations
(1830) Pogson
Named after
Norman Pogson[2]
(English astronomer)
1968 HA · 1926 GW
1929 EE · 1942 EC1
1945 BB · 1953 RE1
1955 FX · 1955 GE
1961 AC · 1969 QM
1971 BJ · 1972 NA1
1972 OC · 1972 OD
main-belt[1][3] · (inner)
Flora[4][5] · binary[5][6][7]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc92.52yr (33,794 d)
Aphelion2.3117AU
Perihelion2.0652 AU
2.1884 AU
Eccentricity0.0563
3.24 yr (1,182 d)
342.96°
0° 18m 15.84s / day
Inclination3.9540°
147.45°
334.96°
Knownsatellites1(D: 2.52 km,P: 24.24 h)[5][6][7]
Physical characteristics
7.710±0.669 km[8][9]
8.284±0.116 km[10]
8.35 km[11]
2.56999±0.00004 h[12]
0.2188[11]
0.2361[10]
0.274[8][9]
Tholen =S[4]
SMASS =S[4][5]
B–V = 0.910[4]
U–B = 0.500[4]
12.45[1][3]
12.61[8][10]

1830 Pogson, provisional designation1968 HA, is a stonyFlorian asteroid and an asynchronousbinary system from the inner regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 17 April 1968, by Swiss astronomerPaul Wild at theZimmerwald Observatory near Bern, Switzerland.[1] TheS-type asteroid has arotation period 2.6 of hours.[5] It was named for English astronomerNorman Pogson. The discovery of its 2.5-kilometer sizedcompanion was announced in May 2007.[6][7]

Orbit and classification

[edit]

According to aHCM-analysis byDavid Nesvorný,Pogson is a member of theFlora family (402),[4] a giantasteroid clan and the largestfamily of stony asteroids in the asteroid belt.[5][13] It has also been grouped into theAugusta family (list) byZappalà, while forMilani andKnežević, who don't recognize the Florian clan as a family,Pogson is a non-family asteroid from the main belt'sbackground population.[14]

It orbits the Sun in theinner asteroid belt at a distance of 2.1–2.3 AU once every 3 years and 3 months (1,182 days;semi-major axis of 2.19 AU). Its orbit has aneccentricity of 0.06 and aninclination of 4° with respect to theecliptic.[3] The asteroid was first observed as1926 GW atSimeiz Observatory in April 1926. The body'sobservation arc begins with its observation as1929 EE atHeidelberg Observatory in March 1929, or 39 years prior to its official discovery observation atZimmerwald.[1]

Naming

[edit]

Thisminor planet was named after English astronomerNorman Pogson (1829–1891), inventor of the modern astronomicalmagnitude scale. At theRadcliffe andMadras observatories, he discovered eight asteroids, including42 Isis and67 Asia.[2] The officialnaming citation was published by theMinor Planet Center on 15 October 1977 (M.P.C. 4236).[15] The lunar craterPogson was also named in his honor.[2]

Physical characteristics

[edit]

In theTholen andSMASS classification,Pogson is a common, stonyS-type asteroid.[3]

Rotation period

[edit]

In April 2007, a rotationallightcurve ofPogson was obtained fromphotometric observations by an international collaboration of Australian, European and American astronomers, namely,David Higgins,Petr Pravec,Peter Kušnirák,Julian Oey andDonald Pray. Lightcurve analysis gave arotation period of2.5702±0.0001 hours with a brightness variation of 0.12magnitude (U=3).[7] In the following month, a more refined period of2.56990±0.00004 hours with the same amplitude was measured by Petr Pravec (U=3).[12]

Additional period determinations were made by Melissa Dykhuis and collaborators (2.5698 h) at the Calvin College Observatory (H62) during 2008 (U=2+),[16] and byPierre Antonini (2.5699 h) and Julian Oey (2.604 h) in March 2013 (U=3-/2).[17][18]

Satellite

[edit]

During the photometric observation in 2007, it was also revealed, thatPogson is an asynchronousbinary system with aminor-planet moon in its orbit.[7] The mutual eclipse andoccultation events showed that the companion orbits its primary every 24.24 hours.[7][12] Based on a secondary-to-primary diameter ratio of 0.32 or larger, Johnston's archive estimates a diameter of 2.52 kilometers for the satellite, separated by 8 kilometers from its primary.[6]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Pogson measures between 7.7 and 8.35 kilometers in diameter and its surface has analbedo between 0.2188 and 0.274.[8][9][10][11] TheCollaborative Asteroid Lightcurve Link adopts the result from Petr Pravec's revised WISE-data,[11] that is, an albedo of 0.2188 and a diameter of 8.35 kilometers based on anabsolute magnitude of 12.659.[5]

References

[edit]
  1. ^abcde"1830 Pogson (1968 HA)".Minor Planet Center. Retrieved7 December 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(1830) Pogson".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 147.doi:10.1007/978-3-540-29925-7_1831.ISBN 978-3-540-00238-3.
  3. ^abcde"JPL Small-Body Database Browser: 1830 Pogson (1968 HA)" (2018-10-22 last obs.).Jet Propulsion Laboratory. Retrieved7 December 2018.
  4. ^abcdef"Asteroid 1830 Pogson".Small Bodies Data Ferret. Retrieved7 December 2018.
  5. ^abcdefg"LCDB Data for (1830) Pogson". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2018.
  6. ^abcdJohnston, Wm. Robert (21 September 2014)."Asteroids with Satellites Database – (1830) Pogson".Johnston's Archive. Retrieved7 December 2018.
  7. ^abcdefHiggins, D.; Pravec, P.; Kusnirak, P.; Oey, J.; Pray, D. (May 2007)."(1830) Pogson".Central Bureau Electronic Telegrams.957 (957): 1.Bibcode:2007CBET..957....1H. Retrieved7 December 2018.
  8. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved7 December 2018.
  9. ^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.S2CID 119293330.
  10. ^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. (catalog)
  11. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  12. ^abcPravec, P.; Scheirich, P.; Vokrouhlický, D.; Harris, A. W.; Kusnirák, P.; Hornoch, K.; et al. (March 2012). "Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries".Icarus.218 (1):125–143.Bibcode:2012Icar..218..125P.doi:10.1016/j.icarus.2011.11.026.
  13. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.S2CID 119280014.
  14. ^"Asteroid (1830) Pogson – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved4 December 2018.
  15. ^Schmadel, Lutz D. (2009)."Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.
  16. ^Dykhuis, Melissa J.; Molnar, Lawrence A.; Gates, Christopher J.; Gonzales, Joshua A.; Huffman, Jared J.; Maat, Aaron R.; et al. (March 2016). "Efficient spin sense determination of Flora-region asteroids via the epoch method".Icarus.267:174–203.Bibcode:2016Icar..267..174D.doi:10.1016/j.icarus.2015.12.021.
  17. ^Behrend, Raoul."Asteroids and comets rotation curves – (1830) Pogson". Geneva Observatory. Retrieved7 December 2018.
  18. ^Oey, Julian (October 2014). "Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2013".The Minor Planet Bulletin.41 (4):276–281.Bibcode:2014MPBu...41..276O.ISSN 1052-8091.

External links

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