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1652 Hergé

From Wikipedia, the free encyclopedia
Asteroid

1652 Hergé
Shape model ofHergé from itslightcurve
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date9 August 1953
Designations
(1652) Hergé
Named after
Georges Remi
(Hergé)cartoonist[2]
1953 PA · 1933 UE1
1939 HG
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.41 yr (30,464 days)
Aphelion2.5883AU
Perihelion1.9139 AU
2.2511 AU
Eccentricity0.1498
3.38yr (1,234 days)
34.960°
Inclination3.1989°
251.72°
13.107°
Physical characteristics
Dimensions8.689±0.081 km[4]
8.954±0.083 km[5]
9.41 km(calculated)[3]
16.36±0.02h[a][b]
0.1160±0.0215[5]
0.137±0.028[6]
0.24(assumed)[3]
0.308±0.060[4]
S[3][7]
12.20[4] · 12.3[1][3] · 12.54±0.19[7] · 13.2[5]

1652 Hergé, provisional designation1953 PA, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 9 August 1953, by Belgian astronomerSylvain Arend at theRoyal Observatory of Belgium in Uccle, Belgium.[8] It was later named after Belgian cartoonistHergé.[2]

Orbit and classification

[edit]

Hergé is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,234 days). Its orbit has aneccentricity of 0.15 and aninclination of 3° with respect to theecliptic.[1] It was first identified as1933 UE1 atHeidelberg Observatory in 1933, extending the body'sobservation arc by 20 years prior to its official discovery observation.[8]

Physical characteristics

[edit]

Hergé has been characterized as a commonS-type asteroid byPan-STARRS photometric survey.[7]

Rotation period

[edit]

AstronomerPetr Pravec obtained a rotationallightcurve ofHergé from photometric observations taken atOndřejov Observatory in September 2014.[b] It gave arotation period of 16.36 hours with a brightness amplitude of 0.42magnitude (U=3-).[a]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Hergé measures between 8.68 and 8.95 kilometers in diameter, and its surface has analbedo between 0.116 and 0.308.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 9.41 kilometers with anabsolute magnitude of 12.54.[3]

Naming

[edit]

Thisminor planet was named in honor of Belgian cartoonistGeorges Remi, better known under his pseudonym Hergé. He is considered to be the father of the fictionalAdventures of Tintin, one of the most popular European comics of the 20th century, and creator of its hero,Tintin, in 1929.[2] The asteroid1683 Castafiore was also named after the comic-strip characterBianca Castafiore from the series. The approved naming citation was published by theMinor Planet Center on 8 April 1982 (M.P.C. 6831).[9]

Notes

[edit]
  1. ^abPravec (2014) web (2014-09-18): rotation period of16.36±0.02, 0.42 mag, (quality code of 3-). Summary figures for (1652) Herge atAsteroid Lightcurve Database andPravec, P.; Wolf, M.; Sarounova, L. (2014)
  2. ^ablightcurve plot of (1652) Hergé. Lightcurve analysis by Petr Pravec

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1652 Herge (1953 PA)" (2017-03-16 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1652) Hergé".Dictionary of Minor Planet Names – (1652) Hergé.Springer Berlin Heidelberg. p. 131.doi:10.1007/978-3-540-29925-7_1653.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1652) Hergé". Asteroid Lightcurve Database (LCDB). Retrieved25 December 2016.
  4. ^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. Retrieved25 December 2016.
  5. ^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.
  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. Retrieved25 December 2016.
  7. ^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. Retrieved25 December 2016.
  8. ^ab"1652 Herge (1953 PA)".Minor Planet Center. Retrieved25 December 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 December 2016.

External links

[edit]
Minor planets
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Authority control databasesEdit this at Wikidata
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