Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1434 Margot

From Wikipedia, the free encyclopedia
Main-belt asteroid

1434 Margot
Discovery[1]
Discovered byG. Neujmin
Discovery siteSimeiz Obs.
Discovery date19 March 1936
Designations
(1434) Margot
Named after
Gertrud Margot Görsdorf[2]
(friend ofWilhelm Gliese)
1936 FD1 · 1931 GM
1931 HA · 1938 RD
1938 UN · 1988 DU
A906 QA · A922 SD
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.11 yr (40,582 days)
Aphelion3.2158AU
Perihelion2.8217 AU
3.0187 AU
Eccentricity0.0653
5.24yr (1,916 days)
86.589°
0° 11m 16.44s / day
Inclination10.832°
152.42°
147.81°
Physical characteristics
Dimensions27.178±0.303 km[5]
27.20±1.75 km[6]
28.052±0.039 km[7]
29.49 km(derived)[3]
29.65±1.4 km[8]
30.84±0.62 km[9]
8.17h[10]
0.1106(derived)[3]
0.117±0.249[6]
0.1242±0.0101[7]
0.130±0.023[5]
0.132±0.006[9]
0.1353±0.013[8]
Tholen =S[1][3] · S[11]
B–V = 0.809[1]
U–B = 0.404[1]
10.43[1][9][8] · 10.49±0.05[11] · 10.66[10][7][3] · 10.77[6]

1434 Margot, provisional designation1936 FD1, is a stony Eoanasteroid from the outer regions of theasteroid belt, approximately 29 kilometers in diameter. It was discovered on 19 March 1936, by Soviet astronomerGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula.[12] The asteroid was named after Gertrud Margot Görsdorf, a friend of German astronomer ofWilhelm Gliese.[2]

Orbit and classification

[edit]

Margot is a member theEos family (606),[3][4] the largestasteroid family of theouter asteroid belt consisting of nearly 10,000 asteroids.[13]: 23  It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,916 days). Its orbit has aneccentricity of 0.07 and aninclination of 11° with respect to theecliptic.[1]

The body'sobservation arc begins atVienna Observatory in August 1906, when it was first identified asA922 SD, almost 30 years prior to its official discovery observation at Simeiz.[12]

Physical characteristics

[edit]

In theTholen classification,Margot is a commonS-type asteroid.[1][3]Pan-STARRS photometric survey also characterizes it as a stony S-type,[11] while the overallspectral type for Eoan asteroids is that of aK-type.[13]: 23 

Rotation period

[edit]

In June 1984, a rotationallightcurve ofMargot was obtained from photometric observations by American astronomerRichard Binzel . Lightcurve analysis gave a well-definedrotation period of 8.17 hours with a brightness amplitude of 0.52magnitude, indicative of a somewhat elongated shape (U=3).[10]

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,Margot measures between 27.178 and 30.84 kilometers in diameter and its surface has analbedo between 0.117 and 0.1353.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1106 and a diameter of 29.49 kilometers based on anabsolute magnitude of 10.66.[3]

Naming

[edit]

Thisminor planet was named by German astronomerWilhelm Gliese after Gertrud Margot Zottmann (1915–1990; née Görsdorf), his friend and schoolfellow for several years at Berlin. Gliese, after whom the asteroid(1823) is named, is best known for theGliese Catalogue of Nearby Stars, which is itself the source of name for many discoveredexoplanets.[2] The discovery circumstances and naming were researched byLutz Schmadel, the author of theDictionary of Minor Planet Names.[2]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1434 Margot (1936 FD1)" (2017-09-30 last obs.).Jet Propulsion Laboratory. Retrieved24 October 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1434) Margot".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 115.doi:10.1007/978-3-540-29925-7_1435.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1434) Margot". Asteroid Lightcurve Database (LCDB). Retrieved24 October 2017.
  4. ^ab"Asteroid 1434 Margot – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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. Retrieved24 October 2017.
  6. ^abcdMasiero, 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. Retrieved24 October 2017.
  7. ^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.
  8. ^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.
  9. ^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)
  10. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved24 October 2017.
  11. ^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. Retrieved24 October 2017.
  12. ^ab"1434 Margot (1936 FD1)".Minor Planet Center. Retrieved24 October 2017.
  13. ^abNesvorný, 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.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1434_Margot&oldid=1313076849"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp