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(7335) 1989 JA

From Wikipedia, the free encyclopedia
Near-Earth asteroid in 2022

(7335) 1989 JA
Radar images of 1989 JA and its satellite, imaged by theGoldstone observatory in May 2022
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date1 May 1989
Designations
(7335) 1989 JA
1989 JA
Apollo · NEO · PHA[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.98 yr (10,221 days)
Aphelion2.6277AU
Perihelion0.9136 AU
1.7706 AU
Eccentricity0.4840
2.36yr (861 days)
341.87°
0° 25m 5.88s / day
Inclination15.196°
61.325°
232.24°
Earth MOID0.0225 AU · 8.8LD
Physical characteristics
Dimensions0.932±0.153 km[2]
1.18 km(calculated)[3]
1.8 km(outdated)[1]
<12h[4]
0.20(assumed)[3]
0.31±0.30[3][5]
0.322±0.150[2][6]
S[3]
17.0[1][2][3] · 17.8±0.3[7]

(7335) 1989 JA (provisional designation1989 JA) is a stonyasteroid of theApollo group, classified asnear-Earth object andpotentially hazardous asteroid, approximately 1 kilometer in diameter. It was discovered on 1 May 1989, by American astronomerEleanor Helin at the U.S.Palomar Observatory in California.[8] On 27 May 2022, the asteroid made a close approach 0.027astronomical units (4.0×10^6 km; 2.5×10^6 mi) from Earth. During the close approach, optical observations detected signs of an orbitingsatellite, which was later confirmed by radar imaging at NASA'sGoldstone Solar System Radar in California.[9]

2022 close approach[1]
DateJPL SBDB
nominal geocentric
distance
uncertainty
region
(3-sigma)
2022-05-274024703 km± 153 km

Orbit and classification

[edit]

TheS-type asteroid orbits the Sun at a distance of 0.9–2.6 AU once every 2 years and 4 months (861 days). Its orbit has aneccentricity of 0.48 and aninclination of 15° with respect to theecliptic.[1] The first observation was made at the discovering observatory in April 1989, extending the asteroid'sobservation arc by 1 month prior to its discovery observation.[8] It has aminimum orbital intersection distance to Earth of 0.0225 AU (3,370,000 km) which corresponds to 8.8lunar distances.[1]

Physical characteristics

[edit]

During its discovery in May 1989,radiometric observations for this asteroid atArecibo andGoldstone Observatory rendered arotation period of less than 12 hours (U=n.a.).[4] According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 0.93 kilometers in diameter and its surface has a highalbedo of 0.31–0.32,[2][5][6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.18 kilometers, based on an absolute magnitude of 17.0.[3]

Naming

[edit]

As of 2022,1989 JA remains unnamed.[8]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 7335 (1989 JA)" (2017-03-31 last obs.).Jet Propulsion Laboratory. Retrieved26 May 2017.
  2. ^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.
  3. ^abcdef"LCDB Data for (7335)". Asteroid Lightcurve Database (LCDB). Retrieved26 September 2016.
  4. ^abMahapatra, Pravas R.; Benner, Lance A. M.; Ostro, Steven J.; Jurgens, Raymond F.; Giorgini, Jon D.; Yeomans, Donald K.; et al. (March 2002)."Radar observations of asteroid 7335 ( 1989 JA)".Planetary and Space Science.50 (3):257–260.Bibcode:2002P&SS...50..257M.doi:10.1016/S0032-0633(02)00002-8. Retrieved26 September 2016.
  5. ^abMainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Wright, E.; Cutri, R. M.; et al. (August 2011)."Thermal Model Calibration for Minor Planets Observed with Wide-field Infrared Survey Explorer/NEOWISE".The Astrophysical Journal.736 (2): 9.Bibcode:2011ApJ...736..100M.CiteSeerX 10.1.1.472.4936.doi:10.1088/0004-637X/736/2/100. Retrieved26 September 2016.
  6. ^abMainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011)."NEOWISE Observations of Near-Earth Objects: Preliminary Results".The Astrophysical Journal.743 (2): 17.arXiv:1109.6400.Bibcode:2011ApJ...743..156M.doi:10.1088/0004-637X/743/2/156. Retrieved26 September 2016.
  7. ^Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved26 September 2016.
  8. ^abc"7335 (1989 JA)".Minor Planet Center. Retrieved26 September 2016.
  9. ^Benner, Lance A. M."Goldstone Radar Observations Planning: (7335) 1989 JA, 388945 2008 TZ3, and 467460 2006 JF42".Asteroid Radar Research. Jet Propulsion Laboratory. Retrieved15 June 2022.

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