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1719 Jens

From Wikipedia, the free encyclopedia
Main-belt asteroid

1719 Jens
Shape model ofJens from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date17 February 1950
Designations
(1719) Jens
Named after
Jens(discoverer's grandson)[2]
1950 DP · 1939 PP
1939 TD · 1941 BB
1948 RQ · 1948 RS1
1948 TS1 · 1961 TZ1
A922 SC
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.65 yr (25,074 days)
Aphelion3.2474AU
Perihelion2.0649 AU
2.6562 AU
Eccentricity0.2226
4.33yr (1,581 days)
321.62°
0° 13m 39.72s / day
Inclination14.281°
323.44°
58.096°
Physical characteristics
Dimensions18.76 km(derived)[3]
18.93±0.9 km[4]
19.77±0.76 km[5]
19.914±0.070 km[6]
21.610±0.086[7]
5.867±0.005h[8]
5.87±0.01 h[9]
5.87016±0.00005 h[10]
5.873±0.005 h[11]
0.085±0.011[7]
0.1048(derived)[3]
0.1348±0.0306[6]
0.137±0.021[5]
0.1489±0.015[4]
C[12] · S[3]
11.3[4][5][6] · 11.7[1][3] · 12.04±1.20[12]

1719 Jens (prov. designation:1950 DP) is abackground asteroid from the central region of theasteroid belt, approximately 19 kilometers in diameter. It was discovered on 17 February 1950, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[13] It was named after a grandson of the discoverer.[2]

Orbit and classification

[edit]
Jens (yellow-green dots) transists near the center of the Tadpole Nebula.

Jens orbits the Sun in thecentral main-belt at a distance of 2.1–3.2 AU once every 4 years and 4 months (1,581 days). Its orbit has aneccentricity of 0.22 and aninclination of 14° with respect to theecliptic.[1] First identified asA922 SC atSimeiz Observatory in 1922,Jens's first used observation was taken atTurku in 1948, extending the body'sobservation arc by 2 years prior to its official discovery observation.[13]

In 2010,Jens was passing in front of the Tadpole Nebula(see image obtained byWISE).[14]

Physical characteristics

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Lightcurves

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In September 2000, American astronomerBrian Warner obtained two rotationallightcurves, giving arotation period of 5.867 and 5.87 hours with a brightness variation of 0.50 and 0.55magnitude, respectively (U=3/3).[8][9]

In February 2006, photometric observations by French amateur astronomerLaurent Bernasconi gave a concurring period of 5.873 hours with an amplitude of 0.55 magnitude (U=3).[11] This well-defined period was further confirmed by a modeled light-curve using data from the Lowell Photometric Database, giving a period of 5.87016 hours (U=n.a.).[10]

Spectral type

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It is classified asS- andC-type asteroid by the LCDB andPan-STARRS, respectively.[3][12]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Jens measures between 18.93 and 21.61 kilometers in diameter and its surface has analbedo between 0.085 and 0.149.[4][5][6] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1048 and calculates a diameter of 18.76 kilometers based on an absolute magnitude of 11.7.[3]

Naming

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Thisminor planet was named by the discoverer for his grandson. Karl Reinmuth also named the consecutively numbered asteroid,1720 Niels, after one of his grandsons.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3933).[15]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1719 Jens (1950 DP)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved7 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1719) Jens".Dictionary of Minor Planet Names – (1719) Jens.Springer Berlin Heidelberg. p. 136.doi:10.1007/978-3-540-29925-7_1720.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1719) Jens". Asteroid Lightcurve Database (LCDB). Retrieved22 December 2016.
  4. ^abcdTedesco, 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.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  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. Retrieved22 December 2016.
  6. ^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.
  7. ^abMasiero, 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. Retrieved22 December 2016.
  8. ^abWarner, B. (March 2001)."Asteroid Photometry at the Palmer Divide Observatory: Results for 706 Hirundo, 957 Camelia, and 1719 Jens".The Minor Planet Bulletin.28:4–5.Bibcode:2001MPBu...28....4W. Retrieved22 December 2016.
  9. ^abWarner, Brian D. (January 2011)."Upon Further Review: V. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory".The Minor Planet Bulletin.38 (1):63–65.Bibcode:2011MPBu...38...63W.ISSN 1052-8091. Retrieved22 December 2016.
  10. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved22 December 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1719) Jens".Geneva Observatory. Retrieved22 December 2016.
  12. ^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. Retrieved22 December 2016.
  13. ^ab"1719 Jens (1950 DP)".Minor Planet Center. Retrieved22 December 2016.
  14. ^"Asteroid Caught Marching Across Tadpole Nebula".JPL Photojournal. 13 May 2010. Retrieved15 November 2015.
  15. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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