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14827 Hypnos

From Wikipedia, the free encyclopedia
Asteroid

14827 Hypnos
Discovery[1]
Discovered byC. S. Shoemaker
E. M. Shoemaker
Discovery sitePalomar Obs.
Discovery date5 May 1986
Designations
(14827) Hypnos
Pronunciation/ˈhɪpnɒs/
Named after
Hypnos[2]
(Greek god of sleep)
1986 JK
Apollo · NEO · PHA[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc19.32 yr (7,058 days)
Aphelion4.7318AU
Perihelion0.9491 AU
2.8405 AU
Eccentricity0.6659
4.79yr (1,749 days)
206.81°
0° 12m 21.24s / day
Inclination1.9808°
57.976°
238.09°
Earth MOID0.0147 AU · 5.7LD
Jupiter MOID0.5249 AU
Physical characteristics
0.520±0.260 km[4]
>0.74 km[5]
0.9 km(Gehrels 1994)[1]
0.907 km(derived)[6]
0.057(assumed)[6]
<0.067(radar)[5]
0.22±0.17[4]
C[5][6]
B–V = 0.684[1]
U–B = 0.492[1]
18.3[1] · 18.65±0.22[4] · 18.94[6][7]

14827 Hypnos (provisional designation:1986 JK) is a highly eccentric, sub-kilometer-sized carbonaceousasteroid that is thought to be anextinct comet. It is classified asnear-Earth object andpotentially hazardous asteroid of theApollo group.

The asteroid was discovered by American astronomer coupleCarolyn andEugene Shoemaker at thePalomar Observatory in California on 5 May 1986.[3] It was named afterHypnos, the Greek god of sleep.[2]

Orbit and classification

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Comet-like orbit of Hypnos with a higheccentricity of 0.67

Hypnos orbits the Sun at a distance of 0.9–4.7 AU once every 4 years and 9 months (1,749 days). Its orbit has a higheccentricity of 0.67 and aninclination of 2° with respect to theecliptic.[1] It is frequentlyperturbed byJupiter.[8]

The body'sobservation arc begins atAnderson Mesa Station the night prior to its official discovery observation at Palomar.[3]

Close approaches

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As anear-Earth object andpotentially hazardous asteroid Hypnos has an Earthminimum orbital intersection distance of 0.0147 AU (2,200,000 km), which corresponds to 5.7lunar distances.[1]

In 1958, Hypnos passed less than 0.03 AU from both Earth and Mars.[9] Neither planet has been approached so closely by Hypnos since the 862 AD pass of Earth, or will be until the 2214 pass of Earth.[citation needed] It is also aMars-crosser.

Extinct comet

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Hypnos may be thenucleus of anextinct comet that is covered by a crust several centimeters thick that prevents any remainingvolatiles fromoutgassing.[10]

Physical characteristics

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Hypnos is an assumed carbonaceousC-type asteroid.[6][5]

Lightcurves

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As of 2018, no rotationallightcurve of Hypnos has been obtained from photometric observations. The asteroidsrotation period andspin axis remains unknown.[6] It has a low brightness amplitude of 0.05magnitude which indicates that the body has a ratherspheroidal shape.[7]

Diameter and albedo

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According to the NEOSurvey carried out by NASA'sSpitzer Space Telescope, Hypnos measures 520 meters in diameter and its surface has analbedo of 0.22 based on anabsolute magnitude of 18.65,[4] while infrared radiometry gave a radar albedo of no more than 0.067 and a diameter of at least 740 meters.[5]

TheCollaborative Asteroid Lightcurve Link assumes a standard optical albedo for carbonaceous asteroids 0.057 and derives a diameter of 907 meters with anabsolute magnitude of 18.94.[6] The diameter agrees withTom Gehrels 1994-publicationHazards due to Comets and Asteroids in which he estimated amean diameter of 900 meters for Hypnos.[1]

Naming

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Thisminor planet was named afterHypnos fromGreek mythology. He is the god of sleep, son ofNyx andErebus and twin brother ofThanatos. He enters the sleep of mortals and gives them dreams of foolishness or inspiration.[2] The English word "hypnosis" is derived from his name. The official naming citation was published by theMinor Planet Center on 6 January 2003 (M.P.C. 47301).[11]

Exploration

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Hypnos was a potential target for theLICIACube extended mission,[12] but contact was lost shortly after completion of the primary mission.

References

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  1. ^abcdefghij"JPL Small-Body Database Browser: 14827 Hypnos (1986 JK)" (2005-08-30 last obs.).Jet Propulsion Laboratory. Retrieved12 September 2017.
  2. ^abcSchmadel, Lutz D. (2006). "(14827) Hypnos [2.84, 0.67, 2.0]".Dictionary of Minor Planet Names – (14827) Hypnos, Addendum to Fifth Edition: 2003–2005.Springer Berlin Heidelberg. p. 88.doi:10.1007/978-3-540-34361-5_896.ISBN 978-3-540-34361-5.
  3. ^abc"14827 Hypnos (1986 JK)".Minor Planet Center. Retrieved12 September 2017.
  4. ^abcdTrilling, David E.; Mommert, Michael; Hora, Joseph; Chesley, Steve; Emery, Joshua; Fazio, Giovanni; et al. (December 2016)."NEOSurvey 1: Initial Results from the Warm Spitzer Exploration Science Survey of Near-Earth Object Properties".The Astronomical Journal.152 (6): 10.arXiv:1608.03673.Bibcode:2016AJ....152..172T.doi:10.3847/0004-6256/152/6/172.
  5. ^abcdeLance Benner (3 April 2012)."NEA Radar Albedo Ranking". Asteroid Radar Research. Archived fromthe original on 6 October 2000. Retrieved12 September 2017.
  6. ^abcdefg"LCDB Data for (14827) Hypnos". Asteroid Lightcurve Database (LCDB). Retrieved12 September 2017.
  7. ^abWisniewski, W. Z. (June 1987)."Photometry of six radar target asteroids".Icarus.70 (3):566–572.Bibcode:1987Icar...70..566W.doi:10.1016/0019-1035(87)90096-0.ISSN 0019-1035. Retrieved12 September 2017.
  8. ^"JPL Close-Approach Data: 14827 Hypnos (1986 JK)" (last observation: 2000-10-25). Retrieved6 May 2009.
  9. ^"NEODys (14827) Hypnos". Department of Mathematics, University of Pisa. Retrieved12 September 2017.
  10. ^Whitman, Kathryn; Morbidelli, Alessandro; Jedicke, Robert (July 2006)."The size frequency distribution of dormant Jupiter family comets".Icarus.183 (1):101–114.arXiv:astro-ph/0603106.Bibcode:2006Icar..183..101W.CiteSeerX 10.1.1.256.3946.doi:10.1016/j.icarus.2006.02.016.S2CID 14026673. Retrieved12 September 2017.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved12 September 2017.
  12. ^https://twitter.com/LICIACube/status/1585556947595661313/photo/1[bare URL]

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
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