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7088 Ishtar

From Wikipedia, the free encyclopedia
Asteroid named after goddess Ishtar

7088 Ishtar
Discovery[1]
Discovered byC. Shoemaker
Discovery sitePalomar Obs.
Discovery date1 January 1992
Designations
(7088) Ishtar
Pronunciation/ˈɪʃtɑːr/[2]
Named after
Ishtar[1]
(Mesopotamian goddess)
1992 AA
NEO · Amor[1][3]
Binary[4][5]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc38.52yr (14,071 d)
Aphelion2.7551AU
Perihelion1.2057 AU
1.9804 AU
Eccentricity0.3912
2.79 yr (1,018 d)
284.83°
0° 21m 12.96s / day
Inclination8.3045°
102.65°
354.73°
Knownsatellites1[4][5]
(P:20.65 h;D: 330 m)[4][6][7]
Earth MOID0.2230 AU (86.9LD)
Physical characteristics
1.298±0.261 km(primary)[8]
1.51 km(effective)[9]
2.6790±0.0002 h[6][7]
0.260±0.122[8]
U[10]
16.7[1]
16.80[3][8]

7088 Ishtar, provisional designation1992 AA, is a synchronousbinary asteroid andnear-Earth object from theAmor group, approximately 1.3 kilometers (0.81 miles) in diameter. It was discovered on 1 January 1992, by American astronomerCarolyn Shoemaker at thePalomar Observatory in California.[1] The relatively bright asteroid with an unknownspectral type has arotation period of 2.7 hours.[10][11] In December 2005, a 330-meter sizedsatellite was discovered,orbiting its primary every 20.65 hours.[6]

Orbit and classification

[edit]

Ishtar orbits the Sun at a distance of 1.2–2.8 AU once every 2 years and 9 months (1,018 days;semi-major axis of 1.98 AU). Its orbit has aneccentricity of 0.39 and aninclination of 8° with respect to theecliptic.[3] The body'sobservation arc begins with its first observation at theSiding Spring Observatory in March 1981, almost 11 years prior to its official discovery observation atPalomar.[1]

Naming

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Thisminor planet was named after the ancient Mesopotamian goddessIshtar (Inanna). She is the principal goddess of the Assyrians and Babylonians associated with love, fertility, sex and war. The officialnaming citation was published by theMinor Planet Center on 22 April 1997 (M.P.C. 29671).[12]

Physical characteristics

[edit]

Ishtar has an unknownspectral type (U).[10] TheCollaborative Asteroid Lightcurve Link (CALL) assumes standardS-type asteroid due to its relatively high albedo(see below).[11]

Rotation period

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In December 2005, a rotationallightcurve ofIshtar was obtained fromphotometric observations byVishnu Reddy and collaborators. Lightcurve analysis gave arotation period of2.6790±0.0002 h hours with a brightness amplitude of 0.11magnitude (U=3).[6][7][13]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Ishtar measures 1.298 kilometers in diameter and its surface has analbedo of 0.26.[8][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and derives a diameter of 1.16 kilometers based on anabsolute magnitude of 17.08.[11]

References

[edit]
  1. ^abcdef"7088 Ishtar (1992 AA)".Minor Planet Center. Retrieved5 October 2019.
  2. ^"Ishtar".Lexico UK English Dictionary.Oxford University Press. Archived fromthe original on 22 March 2020.
  3. ^abcd"JPL Small-Body Database Browser: 7088 Ishtar (1992 AA)".Jet Propulsion Laboratory (2019-09-11 last obs.). Retrieved5 October 2019.
  4. ^abcJohnston, Wm. Robert (29 May 2019)."Asteroids with Satellites Database – 7088 Ishtar (1992 AA)".Johnston's Archive. Retrieved5 October 2019.
  5. ^abLance A. M. Benner (18 November 2013)."Binary and Ternary near-Earth Asteroids detected by radar".NASA/JPL Asteroid Radar Research. Archived fromthe original on 8 June 2004. Retrieved1 March 2014.
  6. ^abcdReddy, V.; Dyvig, R.; Pravec, P.; Kusnirak, P. (February 2005). "2005 AB".IAU Circ.8483 (8483): 3.Bibcode:2005IAUC.8483....3R. ((7088) Ishtar,CBET 384)
  7. ^abcdPravec, P.; Scheirich, P.; Kusnirák, P.; Hornoch, K.; Galád, A.; Naidu, S. P.; et al. (March 2016)."Binary asteroid population. 3. Secondary rotations and elongations".Icarus.267:267–295.Bibcode:2016Icar..267..267P.doi:10.1016/j.icarus.2015.12.019.
  8. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.S2CID 45334910.
  9. ^"Asteroid 7088 Ishtar".Small Bodies Data Ferret. Retrieved5 October 2019.
  10. ^abcCarry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry".Icarus.268:340–354.arXiv:1601.02087.Bibcode:2016Icar..268..340C.doi:10.1016/j.icarus.2015.12.047.S2CID 119258489.
  11. ^abc"LCDB Data for (7088) Ishtar".Asteroid Lightcurve Database (LCDB). Retrieved5 October 2019.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved5 October 2019.
  13. ^Reddy, V.; Dyvig, R. R.; Pravec, P.; Kusnirák, P.; Gajdos, S.; Galád, A.; et al. (March 2007)."Photometric Observations of Binary Near-Earth Asteroid (7088) Ishtar and (11405) 1999 CV3"(PDF).38th Lunar and Planetary Science Conference (PDF) (1338): 1239.Bibcode:2007LPI....38.1239R. Retrieved5 October 2019.

External links

[edit]
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