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1353 Maartje

From Wikipedia, the free encyclopedia
Asteroid

1353 Maartje
Modelled shape of Maartje from itslightcurve
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
Discovery date13 February 1935
Designations
(1353) Maartje
Named after
Maartje Mekking [2]
(daughter of Dutch orbit
computer B. G. Mekking)
1935 CU · 1931 ME
1953 TZ2 · A910 LB
A916 QB · A920 JC
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc97.48 yr (35,606 days)
Aphelion3.2988AU
Perihelion2.7210 AU
3.0099 AU
Eccentricity0.0960
5.22yr (1,907 days)
134.16°
0° 11m 19.32s / day
Inclination9.2032°
211.79°
98.471°
Physical characteristics
Dimensions33.75±3.9 km[5]
34.16 km(derived)[3]
37.16±10.25 km[6]
38.13±0.79 km[7]
39.013±0.534 km[8]
39.55±0.68 km[9]
42.175±0.390 km[10]
12h[11]
18 h[11]
22.930±0.001 h(best)[12]
22.98±0.05 h[11]
22.9924±0.0002 h[13][a]
22.9926 h[14]
0.0687±0.0045[10]
0.088±0.004[7]
0.1073±0.030[5]
0.13±0.06[6]
0.136±0.015[9]
0.1660(derived)[3]
LS[15] · S(assumed)[3]
9.80[9] · 9.9[3] · 10.0[1] · 10.01[6] · 10.01±0.09[15] · 10.40[5][7][10]

1353 Maartje, provisional designation1935 CU, is an Eoanasteroid from the outer regions of theasteroid belt, approximately 37 kilometers in diameter. It was discovered on 13 February 1935, by Dutch astronomerHendrik van Gent at theUnion Observatory in Johannesburg, South Africa.[16] The asteroid was named after Maartje Mekking, daughter of a staff member at the DutchLeiden Observatory.[2]

Orbit and classification

[edit]

Maartje is a member theEos family (606),[3][4] the largestasteroid family in theouter main belt consisting of nearly 10,000 known members.[17]: 23  It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,907 days;semi-major axis of 3.01 AU). Its orbit has aneccentricity of 0.10 and aninclination of 9° with respect to theecliptic.[1]

In June 1910, the asteroid was first identified asA910 LB at theHeidelberg Observatory in Germany, where the body'sobservation arc begins with its identification asA920 JC in May 1920, almost 15 years prior to its official discovery observation at Johannesburg.[16]

Naming

[edit]

Thisminor planet was named after Maartje (Nin) Maria Lindenburg Mekking (1924–2007), daughter of B.G. Mekking (1903–1971), an orbit computer at theLeiden Observatory. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 123).[2]

Physical characteristics

[edit]

Maartje has been characterized as anL- andS-type asteroid byPanSTARRS photometric survey,[15] while the overallspectral type of the Eos family is that of aK-type.[17]: 23 

Rotation period and poles

[edit]
Lightcurve-based 3D-model of Maartje

Several rotationallightcurve of Maartje have been obtained from photometric observations since 2005.[11][12] Lightcurve analysis gave a consolidated, slightly longer-than average, and well-definedrotation period of 22.930 hours with a brightness amplitude between 0.25 and 0.46magnitude (U=3).[3] The asteroid's lightcurve has also been modeled and gave two concurring periods of 22.9924 and 22.9926 hours.[13][14][a] Modeling in 2018 determined twospin axis of (285.0°, 73.0°) and (119.0°, 41.0°) inecliptic coordinates (λ, β).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Maartje measures between 33.75 and 42.175 kilometers in diameter and its surface has analbedo between 0.0687 and 0.136.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1660 and a diameter of 34.16 kilometers based on anabsolute magnitude of 9.9.[3]

Notes

[edit]
  1. ^abUnpublished study (Hanus 2016d). See summary figures for (1353) Maartje at theLCDB

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1353 Maartje (1935 CU)" (2017-11-02 last obs.).Jet Propulsion Laboratory. Retrieved15 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1353) Maartje".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 110.doi:10.1007/978-3-540-29925-7_1354.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1353) Maartje". Asteroid Lightcurve Database (LCDB). Retrieved15 November 2017.
  4. ^ab"Asteroid 1353 Maartje – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  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. ^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. Retrieved15 November 2017.
  9. ^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. Retrieved15 November 2017.
  10. ^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.
  11. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1353) Maartje". Geneva Observatory. Retrieved15 November 2017.
  12. ^abGarceran, Alfonso Carreno; Aznar, Amadeo; Mansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Silva, Alvaro Fornas; et al. (January 2016)."Nineteen Asteroids Lightcurves at Asteroids Observers (OBAS) - MPPD: 2015 April - September".The Minor Planet Bulletin.43 (1):92–97.Bibcode:2016MPBu...43...92G.ISSN 1052-8091. Retrieved15 November 2017.
  13. ^abcHanus, J.; Delbo', M.; Alí-Lagoa, V.; Bolin, B.; Jedicke, R.; Durech, J.; et al. (January 2018). "Spin states of asteroids in the Eos collisional family".Icarus.299:84–96.arXiv:1707.05507.Bibcode:2018Icar..299...84H.doi:10.1016/j.icarus.2017.07.007.
  14. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved15 November 2017.
  15. ^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. Retrieved15 November 2017.
  16. ^ab"1353 Maartje (1935 CU)".Minor Planet Center. Retrieved15 November 2017.
  17. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

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