Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

8013 Gordonmoore

From Wikipedia, the free encyclopedia
Eccentric, stony asteroid and near-Earth object

8013 Gordonmoore
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date18 May 1990
Designations
(8013) Gordonmoore
Named after
Gordon Moore
(Intel co-founder)[2]
1990 KA
NEO · Amor[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.90 yr (23,703 days)
Earliestprecovery date1 September 1951
Aphelion3.1498AU
Perihelion1.2503 AU
2.2000 AU
Eccentricity0.4317
3.26yr (1,192 days)
126.01°
0° 18m 7.2s / day
Inclination7.5685°
105.57°
146.73°
Earth MOID0.2472 AU · 96.3LD
Physical characteristics
Dimensions1.04 km(derived)[4]
2.3 km[1]
6h(dated)[5]
8.40±0.01 h[6]
0.20(assumed)[4]
S[4]
16.67±0.2(R)[4] · 16.9[1] · 17.26±0.149[7] · 17.26[4] · 17.27±0.15[8]

8013 Gordonmoore, provisional designation1990 KA, is an eccentric, stonyasteroid andnear-Earth object of theApollo group, approximately 1–2 kilometers in diameter.

The asteroid was discovered on 18 May 1990, by American astronomerEleanor Helin atPalomar Observatory in California, United States.[3] It was named after Intel co-founderGordon Moore.[2]

Orbit and classification

[edit]

Gordonmoore orbits the Sun at a distance of 1.3–3.1 AU once every 3 years and 3 months (1,192 days). Its orbit has aneccentricity of 0.43 and aninclination of 8° with respect to theecliptic.[1]

It has aminimum orbit intersection distance with Earth of 0.2472 AU (37,000,000 km), or 96.3lunar distance. Due to its eccentric orbit,Gordonmoore is alsoMars-crosser. In 2127, the asteroid will pass the Red Planet within 0.02776 AU (4,150,000 km).[1]

A firstprecovery was taken at the discovering Palomar Observatory in 1951, extending the body'sobservation arc by 39 years prior to its official discovery observation.[3]

Physical characteristics

[edit]

Rotation period

[edit]

In April 2016, a rotationallightcurve ofGordonmoore was obtained from photometric observations by astronomerBrian Warner at the Palmer Divide Station (716) in Colorado. It gave arotation period of8.40 hours with a brightness variation of 0.25magnitude. Lightcurve analysis also gave an alternative period solution of 4.19 hours with an amplitude of 0.25 magnitude. (U=2).[6] The results supersede a previous observations made at theHoher List Observatory in Germany, that gave a shorter period of 6 hours (U=1).[5]

Diameter and albedo

[edit]

TheCollaborative Asteroid Lightcurve Link assumes a standardalbedo forstony asteroids of 0.20 and calculates a diameter of 1.04 kilometers with anabsolute magnitude of 17.26.[4] In the 1990s,Tom Gehrels estimated the body's diameter to be 2.3 kilometers, assuming an albedo of 0.15.[1]

Naming

[edit]

Thisminor planet was named in honour of American entrepreneur and billionaire,Gordon Moore (1929–2023), co-founder ofIntel, known for his revolutionary vision of the future of computers, and author ofMoore's law. As a philanthropist, Moore has supported research and education all his life.[2] The official naming citation was published by theMinor Planet Center on 26 May 2002 (M.P.C. 45747).[9]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 8013 Gordonmoore (1990 KA)" (2016-07-24 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 19 September 2020. Retrieved22 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(8013) Gordonmoore".Dictionary of Minor Planet Names – (8013) Gordonmoore.Springer Berlin Heidelberg. p. 628.doi:10.1007/978-3-540-29925-7_6793.ISBN 978-3-540-00238-3.
  3. ^abc"8013 Gordonmoore (1990 KA)".Minor Planet Center. Retrieved11 August 2016.
  4. ^abcdef"LCDB Data for (8013) Gordonmoore". Asteroid Lightcurve Database (LCDB). Retrieved11 August 2016.
  5. ^abHoffmann, M. (March 1991)."Photometry of 1990 KA".The Minor Planet Bulletin.18: 10.Bibcode:1991MPBu...18...10H. Retrieved11 August 2016.
  6. ^abWarner, Brian D. (October 2016)."Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2016 April-July".The Minor Planet Bulletin.43 (4):311–319.Bibcode:2016MPBu...43..311W.ISSN 1052-8091. Retrieved22 June 2017.
  7. ^Pravec, 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. Retrieved11 August 2016.
  8. ^Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved11 August 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved11 August 2016.

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=8013_Gordonmoore&oldid=1302612189"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp