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5185 Alerossi

From Wikipedia, the free encyclopedia
Main-belt asteroid

5185 Alerossi
Discovery[1]
Discovered byH. E. Holt
Discovery sitePalomar Obs.
Discovery date15 September 1990
Designations
(5185) Alerossi
Named after
Alessandro Rossi
(Italiangeodesist)[2]
1990 RV2 · 1933 SE
1955 SM · 1981 RA1
1984 HG · 1986 UR4
1988 FQ3
main-belt[1][3] · (middle)
background[4][5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc84.34yr (30,804 d)
Aphelion2.8993AU
Perihelion2.4533 AU
2.6763 AU
Eccentricity0.0833
4.38 yr (1,599 d)
34.812°
0° 13m 30.36s / day
Inclination8.3787°
216.42°
216.46°
Physical characteristics
12.86±1.2 km[6][4]
13.36±0.12 km[7]
0.081±0.009[7]
0.1408±0.031[6]
12.6[1][3]

5185 Alerossi (provisional designation1990 RV2) is a backgroundasteroid from the central region of theasteroid belt, approximately 13 miles (21 kilometers) in diameter. It was discovered on 15 September 1990, by American astronomerHenry Holt atPalomar Observatory in California, United States.[1] The asteroid was later named for Italian geodesistAlessandro Rossi.[2]

Orbit and classification

[edit]

Alerossi is a non-family asteroid from the main belt'sbackground population.[4][5] It orbits the Sun in thecentral asteroid belt at a distance of 2.5–2.9 AU once every 4 years and 5 months (1,599 days;semi-major axis of 2.68 AU). Its orbit has aneccentricity of 0.08 and aninclination of 8° with respect to theecliptic.[3]

In 1933, it was first observed as1933 SE atUccle Observatory, extending the body'sobservation arc by 57 years prior to its official discovery observation at Palomar.[1]

Naming

[edit]

Thisminor planet was named after Italian geodesists Alessandro Rossi (born 1964), a member of the "Group of Satellite Flight Dynamics" at the Istituto CNECE in Pisa, Italy. Expert in spacegeodesy and participant in theLaser Geodynamics Satellites (LAGEOS) mission, he examines Earth's artificialorbital debris, the natural debris around mission targets to improve space-craft maneuvers, and the potential hazard ofEarth-crossers.[2] The official naming citation was published by theMinor Planet Center on 28 July 1999 (M.P.C. 61268).[8]

Physical characteristics

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Alerossi measures 12.9 and 13.3 kilometers in diameter and its surface has analbedo of 0.08 and 0.14, respectively.[6][7] It has an absolute magnitude of 12.6.[1][3] As of 2018, the asteroid'sspectral type,rotation period and shape remain unknown.[3][9]

References

[edit]
  1. ^abcdef"5185 Alerossi (1990 RV2)".Minor Planet Center. Retrieved25 July 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(5185) Alerossi".Dictionary of Minor Planet Names – (5185) Alerossi.Springer Berlin Heidelberg. p. 446.doi:10.1007/978-3-540-29925-7_5030.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 5185 Alerossi (1990 RV2)" (2018-01-22 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2018.
  4. ^abc"Asteroid 5185 Alerossi".Small Bodies Data Ferret. Retrieved25 July 2018.
  5. ^ab"Asteroid (5185) Alerossi – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved25 May 2018.
  6. ^abcTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved25 July 2018.
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 May 2016.
  9. ^"LCDB Data for (5185) Alerossi". Asteroid Lightcurve Database (LCDB). Retrieved20 June 2017.

External links

[edit]
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