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5171 Augustesen

From Wikipedia, the free encyclopedia
Main-belt asteroid

5171 Augustesen
Discovery[1]
Discovered byP. Jensen
Discovery siteBrorfelde Obs.
Discovery date25 September 1987
Designations
(5171) Augustesen
Named after
Karl Augustesen[1]
(Danish astronomer)
1987 SQ3 · 1953 RP
1953 RP1 · 1989 CH8
main-belt · (inner)
background[2] · Vestian[3]
Orbital characteristics[4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc64.15yr (23,430 d)
Aphelion2.7460AU
Perihelion2.1036 AU
2.4248 AU
Eccentricity0.1325
3.78 yr (1,379 d)
14.269°
0° 15m 39.6s / day
Inclination7.0844°
322.10°
45.866°
Physical characteristics
6.445±0.074 km[5]
6.81 km(calculated)[3]
9.02±2.21 km[6]
9.41±0.33 km[7]
9.73±2.59 km[8]
19.2±0.1 h(poor)[9]
480±10 h[10][a]
0.08±0.05[6]
0.10±0.06[8]
0.108±0.008[7]
0.20(assumed)[3]
0.245±0.034[5]
X[11] · S[3]
13.10[5][8] · 13.20[3][7]
13.3[4] · 13.52[6]
13.75±0.50[11]

5171 Augustesen (provisional designation1987 SQ3) is a backgroundasteroid andslow rotator from the inner regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 25 September 1987, by Danish astronomerPoul Jensen at theBrorfelde Observatory in Denmark.[1] The suspectedtumbler and presumed Vestian asteroid has an exceptionally slowrotation period of 480 hours and possibly an elongated shape.[3] It was named after Danish astronomerKarl Augustesen.[1]

Orbit and classification

[edit]

Augustesen is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[2] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theVesta family (401), one of the main belt's largestasteroid families named after4 Vesta, the family'sparent body.[3]

It orbits the Sun in theinner main-belt at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,379 days;semi-major axis of 2.42 AU). Its orbit has aneccentricity of 0.13 and aninclination of 7° with respect to theecliptic.[4] The asteroid was first observed as1953 RP and1953 RP1 atHeidelberg andGoethe Link Observatory, where the body'sobservation arc begins in September 1953, or 34 years prior to its official discovery observation at Brorfelde.[1]

Physical characteristics

[edit]

Augustesen has been characterized as anX-type asteroid byPan-STARRS' photometric survey.[11] It is also an assumedS-type asteroid.[3]

Rotation period

[edit]

In October 2006, a rotationallightcurve of Augustesen was obtained from photometric observations by Slovak astronomerAdrián Galád atModra Observatory. Lightcurve analysis gave a longrotation period of 480 hours with a high brightness amplitude of 0.8magnitude, indicative for a non-spherical shape (U=3).[10][a] The asteroid is aslow rotator with a period much longer than the typical 2 to 20 hours measured for most observed asteroids. Augustesen is also a suspectedtumbler with a non-principal axis rotation, also known as "tumbling".[3]

An alternative measurement byLaurent Bernasconi gave a much shorter period based on a fragmentary (poor) lightcurve (U=1).[9]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Augustesen measures between 6.445 and 9.73 kilometers in diameter and its surface has analbedo between 0.08 and 0.245.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.81 kilometers based on anabsolute magnitude of 13.2.[3]

Naming

[edit]

Thisminor planet was named afterKarl Augustesen (born 1945), a Danishastronomer and co-discoverer of minor planets. For several decades he had been an observer using the Schmidt telescope at the discoveringBrorfelde Observatory in Denmark, after which the asteroid3309 Brorfelde was named.[1]

The corrected official naming citation was published by theMinor Planet Center on 22 June 2005 (M.P.C. 54279).[12] In its preceding publication on 23 May 2005, the MPC erroneously named asteroid(6002) 1988 RO, which was discovered by Poul Jensen on 8 September 1988, as "6002 Augustesen" (M.P.C. 54173). As of 2018, theJPL SBDB still shows the (incorrect) discovery date of that other asteroid.[12]

Notes

[edit]
  1. ^abLightcurve plot of (5171) Augustesen (2006) Pravec/Galad. Rotation period480 hours with a brightness amplitude of0.8 mag. Quality code of 3. Summary figures at theLCDB and theOndrejov Asteroid Photometry Project (data sheet).

References

[edit]
  1. ^abcdef"5171 Augustesen (1987 SQ3)".Minor Planet Center. Retrieved26 March 2018.
  2. ^ab"Asteroid 5171 Augustesen – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  3. ^abcdefghij"LCDB Data for (5171) Augustesen". Asteroid Lightcurve Database (LCDB). Retrieved26 March 2018.
  4. ^abc"JPL Small-Body Database Browser: 5171 Augustesen (1987 SQ3)" (2017-10-29 last obs.).Jet Propulsion Laboratory. Retrieved26 March 2018.
  5. ^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.S2CID 46350317. Retrieved26 March 2018.
  6. ^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.
  7. ^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)
  8. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved26 March 2018.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (5171) Augustesen". Geneva Observatory. Retrieved26 March 2018.
  10. ^abGalád, Adrián; Pravec, Petr; Gajdos, Stefan; Kornos, Leonard; Világi, Jozef (October 2007)."Seven Asteroids Studied from Modra Observatory in the Course of Binary Asteroid Photometric Campaign".Earth.101 (1–2):17–25.Bibcode:2007EM&P..101...17G.doi:10.1007/s11038-007-9146-6.S2CID 121779876. Retrieved26 March 2018.
  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.S2CID 53493339. Retrieved26 March 2018.
  12. ^ab"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 March 2018.

External links

[edit]
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Distant minor planet
Comets
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