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3066 McFadden

From Wikipedia, the free encyclopedia
Stony background asteroid from the central regions of the asteroid belt

3066 McFadden
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date1 March 1984
Designations
(3066) McFadden
Named after
Lucy-Ann McFadden[1]
(American astronomer)
1984 EO · 1933 MA
1936 FE · 1941 MA
1952 FW · 1968 FQ
1976 GC · 1980 EG2
main-belt[1][2] · (inner)[3]
background[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc81.60yr (29,806 d)
Aphelion2.8636AU
Perihelion2.1875 AU
2.5255 AU
Eccentricity0.1339
4.01 yr (1,466 d)
328.54°
0° 14m 44.16s / day
Inclination15.574°
175.69°
188.31°
Physical characteristics
13.526±0.046 km[5]
14.805±0.051 km[6]
14.896 km[7]
14.90 km(taken)[3]
15.27±0.53 km[8]
15.63±0.44 km[9]
13.798±0.002 h[10][a]
0.240±0.015[9]
0.2541[7]
0.2617±0.0766[6]
0.275±0.072[8]
0.363±0.033[5]
S(assumed)[3]
11.10[8] · 11.20[2][9]
11.24[3][6]
11.24±0.08[7][11]
11.41±0.25[12]

3066 McFadden, provisional designation1984 EO, is a stony backgroundasteroid from the central regions of theasteroid belt, approximately 15 kilometers (9.3 miles) in diameter. It was discovered on 1 March 1984, by American astronomerEdward Bowell at theAnderson Mesa Station near Tucson, Arizona. It was named for American planetary scientistLucy-Ann McFadden.[1] The assumedS-type asteroid has a rotation period of 13.8 hours.[3][a]

Orbit and classification

[edit]

McFadden is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in thecentral asteroid belt at a distance of 2.2–2.9 AU once every 4 years (1,466 days;semi-major axis of 2.53 AU). Its orbit has aneccentricity of 0.13 and aninclination of 16° with respect to theecliptic.[2]

The asteroid was first observed as1933 MA at theSimeis Observatory in June 1933. The body'sobservation arc begins as1936 FE atUccle Observatory in March 1936, or 48 years prior to its official discovery observation at Anderson Mesa.[1]

Naming

[edit]

Thisminor planet was named afterLucy-Ann McFadden (born 1952), aplanetary scientist at theUniversity of Maryland at the time of naming. Her research included the similarities between the spectra ofmeteorites andnear-Earth objects.[1] The official naming citation was published by theMinor Planet Center on 14 April 1987 (M.P.C. 11748).[13]

Physical characteristics

[edit]

McFadden is an assumed, stonyS-type asteroid.[3]

Rotation period

[edit]

In June 2005, a rotationallightcurve ofMcFadden was obtained from photometric observations by American astronomerBrian Warner at hisPalmer Divide Observatory in Colorado. Lightcurve analysis gave arotation period of 13.798 hours with a brightness amplitude of 0.13magnitude (U=3).[10][a]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,McFadden measures between 13.526 and 15.63 kilometers in diameter and its surface has analbedo between 0.240 and 0.363.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adoptsPetr Pravec's revised WISE data with an albedo of 0.2541 and a diameter of 14.90 kilometers based on anabsolute magnitude of 11.24.[3][7]

Notes

[edit]
  1. ^abcLightcurve plot of 3066 McFadden, Palmer Divide Observatory,B. D. Warner (2005) rotation period of13.798±0.002 hours with a brightness amplitude of0.13±0.02 mag. Quality code of 3. Summary figures at theLCDB and publication.[10]

References

[edit]
  1. ^abcdef"3066 McFadden (1984 EO)".Minor Planet Center. Retrieved27 March 2018.
  2. ^abcd"JPL Small-Body Database Browser: 3066 McFadden (1984 EO)" (2017-10-28 last obs.).Jet Propulsion Laboratory. Retrieved27 March 2018.
  3. ^abcdefg"LCDB Data for (3066) McFadden". Asteroid Lightcurve Database (LCDB). Retrieved27 March 2018.
  4. ^ab"Asteroid 3066 McFadden – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 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.
  6. ^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.
  7. ^abcdePravec, 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.
  8. ^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.
  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. ^abcWarner, Brian D. (December 2005). "Asteroid lightcurve analysis at the Palmer Divide Observatory - spring 2005".The Minor Planet Bulletin.32 (4):90–92.Bibcode:2005MPBu...32...90W.ISSN 1052-8091.
  11. ^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.
  12. ^Veres, 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.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 March 2018.

External links

[edit]
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