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2213 Meeus

From Wikipedia, the free encyclopedia
Main-belt asteroid

2213 Meeus
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date24 September 1935
Designations
(2213) Meeus
Named after
Jean Meeus[1]
(Belgian astronomer)
1935 SO1 · 1958 XM
1961 TG · 1974 RB
main-belt[1][2] · (inner)
background[3] · Flora[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc82.34yr (30,075 d)
Aphelion2.6972AU
Perihelion1.6983 AU
2.1977 AU
Eccentricity0.2273
3.26 yr (1,190 d)
126.11°
0° 18m 9s / day
Inclination5.3321°
126.93°
222.18°
Physical characteristics
4.59±0.28 km[5]
4.889±0.028 km[6]
5.194±0.032 km[7]
5.67 km(calculated)[4]
2.651±0.001 h[8]
0.24(assumed)[4]
0.3467±0.0219[7]
0.439±0.042[5]
S(assumed)[4]
13.12±0.08[8]
13.20[5][7]
13.34±0.36[9]
13.4[2][4]

2213 Meeus, provisional designation1935 SO1, is a bright backgroundasteroid from the inner regions of theasteroid belt, approximately 5 kilometers (3 miles) in diameter. It was discovered on 24 September 1935, by Belgian astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[1] The presumedS-type asteroid has a shortrotation period of 2.65 hours.[4] It was named for Belgian amateur astronomer and meteorologistJean Meeus.[1]

Orbit and classification

[edit]

Meeus is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[4]

It orbits the Sun in theinner main-belt at a distance of 1.7–2.7 AU once every 3 years and 3 months (1,190 days;semi-major axis of 2.2 AU). Its orbit has aneccentricity of 0.23 and aninclination of 5° with respect to theecliptic.[2] The body'sobservation arc begins with its official discovery observation at Uccle in 1935.[1]

Physical characteristics

[edit]

Meeus is an assumed stonyS-type asteroid.[4]

Rotation period

[edit]

In August 2013, a rotationallightcurve ofMeeus was obtained fromphotometric observations by Italian astronomers of the Tuscolana Association of Astronomy (D06). Lightcurve analysis gave arotation period of 2.651 hours with a brightness amplitude of 0.19magnitude (U=3-).[4][8]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Meeus measures between 4.59 and 5.194 kilometers in diameter and its surface has a highalbedo between 0.3467 and 0.439.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 5.67 kilometers based on anabsolute magnitude of 13.4.[4]

Naming

[edit]

Thisminor planet was named after Belgian amateur astronomer and professional meteorologistJean Meeus (born 1928), who, in 1986, received theAmateur Achievement Award of the Astronomical Society of the Pacific.[1] The official naming was proposed by Eric S. Fogelin(see2181),Jay U. Gunter andEdward Bowell, and published by theMinor Planet Center on 1 August 1981 (M.P.C. 6208).[10]

References

[edit]
  1. ^abcdefg"2213 Meeus (1935 SO1)".Minor Planet Center. Retrieved25 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 2213 Meeus (1935 SO1)" (2018-01-26 last obs.).Jet Propulsion Laboratory. Retrieved25 May 2018.
  3. ^ab"Asteroid 2213 Meeus".Small Bodies Data Ferret. Retrieved25 May 2018.
  4. ^abcdefghij"LCDB Data for (2213) Meeus". Asteroid Lightcurve Database (LCDB). Retrieved25 May 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.
  6. ^abMasiero, 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.S2CID 119293330.
  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.S2CID 35447010. (catalog)
  8. ^abcTomassini, Angelo; Cervoni, Maurizio; Scardella, Maurizio (January 2014). "Rotational Period and H-G Parameters for Asteroid 2213 Meeus".The Minor Planet Bulletin.41 (1): 19.Bibcode:2014MPBu...41...19T.ISSN 1052-8091.
  9. ^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.S2CID 53493339.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 May 2018.

External links

[edit]
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