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9965 GNU

From Wikipedia, the free encyclopedia
Asteroid

9965 GNU
Orbits ofGNU (blue), theinner planets andJupiter (outermost)
Discovery[1]
Discovered bySpacewatch
Discovery siteKitt Peak National Obs.
Discovery date5 March 1992
Designations
(9965) GNU
Named after
GNU Project[1]
(free software project)
1992 EF2 · 1988 BD4
1993 QR3
main-belt[1][2] · (inner)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc30.17yr (11,019 d)
Aphelion2.8283AU
Perihelion2.0080 AU
2.4181 AU
Eccentricity0.1696
3.76 yr (1,373 d)
276.39°
0° 15m 43.56s / day
Inclination12.206°
156.48°
82.938°
Physical characteristics
2.07±0.53 km[4]
4.10 km(calculated)[5]
6.22±2.14 km[6]
6.293±0.159 km[7][8]
39.720±0.1589 h(R)[9]
39.745±0.1589 h(S)[9]
0.102±0.014[7]
0.1022±0.0145[8]
0.105±0.125[6]
0.20(assumed)[5]
0.53±0.12[4]
D(Pan-STARRS)[10]
S(SDSS-MOC)[11]
S(assumed)[5]
14.10[6][8]
14.3[2][5]
14.31±0.14[10]
14.398±0.005(R)[9]
14.72[4]
14.966±0.011(S)[9]

9965 GNU, provisional designation1992 EF2, is a backgroundasteroid from the inner regions of theasteroid belt, approximately 4 kilometers (2 miles) in diameter. It was discovered on 5 March 1992, by astronomer of theSpacewatch program at theKitt Peak National Observatory in Arizona, United States.[1] The uncertainD-type asteroid has a longrotation period of 39.7 hours.[5] It was named for the free-softwareGNU Project.[1]

Orbit and classification

[edit]

GNU is a non-family asteroid from the main belt'sbackground population.[3]

It orbits the Sun in theinner asteroid belt at a distance of 2.0–2.8 AU once every 3 years and 9 months (1,373 days;semi-major axis of 2.42 AU). Its orbit has aneccentricity of 0.17 and aninclination of 12° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1988 BD4 atLa Silla Observatory in January 1988, or 4 years prior to its official discovery observation at Kitt Peak.[1]

Physical characteristics

[edit]

GNU has been characterized as a darkD-type asteroid byPan-STARRS' survey and in theSDSS-based taxonomy.[10][11] It is also an assumedS-type asteroid, the most common type in the inner asteroid belt.[5]

Rotation period

[edit]

In September and October 2012, two rotationallightcurves ofGNU were obtained fromphotometric observations by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 39.720 and 39.745 hours, with a brightness amplitude of 0.36 and 0.42magnitude in the R- and S-band, respectively (U=2/2).[9] While not being aslow rotator,GNU' period is significantly longer than the average spin rate of 2 to 20 hours, seen among the majority of asteroids.

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,GNU measures between 2.07 and 6.293 kilometers in diameter and its surface has analbedo between 0.102 and 0.53.[4][6][7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 4.10 kilometers based on anabsolute magnitude of 14.3.[5]

Naming

[edit]

Thisminor planet was named for the free-softwareGNU Project, created byRichard Stallman 1984. GNU is therecursive acronym for "GNU is not Unix". The collaborative projects enables programmers to trade and improve uponfree software.[1] The official naming citation was published by theMinor Planet Center on 11 November 2000 (M.P.C. 41571).[12]

References

[edit]
  1. ^abcdefg"9965 GNU (1992 EF2)".Minor Planet Center. Retrieved28 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 9965 GNU (1992 EF2)" (2018-03-22 last obs.).Jet Propulsion Laboratory. Retrieved28 May 2018.
  3. ^ab"Asteroid 9965 GNU".Small Bodies Data Ferret. Retrieved28 May 2018.
  4. ^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.
  5. ^abcdefg"LCDB Data for (9965) GNU". Asteroid Lightcurve Database (LCDB). Retrieved28 May 2018.
  6. ^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.S2CID 46350317.
  7. ^abcMasiero, 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.S2CID 118745497.
  8. ^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.S2CID 35447010. (catalog)
  9. ^abcdeWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929.
  10. ^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.S2CID 53493339.
  11. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 May 2018.

External links

[edit]
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