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(66063) 1998 RO1

From Wikipedia, the free encyclopedia
Stony near-Earth object of the Aten group

(66063) 1998 RO1
Orbit of1998 RO1
Discovery[1][2]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date14 September 1998
Designations
(66063)1998 RO1
1998 RO1 · 1999 SN5
NEO · Aten[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc13.99 yr (5,111 days)
Aphelion1.7045AU
Perihelion0.2774 AU
0.9910 AU
Eccentricity0.7200
0.99yr (360 days)
348.97°
0° 59m 56.76s / day
Inclination22.678°
351.88°
151.13°
Knownsatellites1(D: 0.38 km;P: 14.53 h)[3][4][5][6]
Earth MOID0.0921 AU · 35.9LD
Physical characteristics
0.62±0.25 km[7]
0.72 km(est. at0.20)[8]
0.8±0.15 km[3][9]
0.860 km(derived)[10]
2.8±1.3 g/cm3[6]
2.4924±0.0003h[4]
2.4924 h[5][9]
0.145[9]
0.30±0.17[7]
S[10][11][12]
18.00[12] · 18.04[9] · 18.05[10] · 18.05±0.071[13] · 18.1[1]

(66063) 1998 RO1 is a stonynear-Earth object of theAten group on a highly-eccentric orbit. The synchronousbinary system measures approximately 800 meters (0.50 miles) in diameter. It was discovered by astronomers of theLincoln Near-Earth Asteroid Research at theLincoln Laboratory's Experimental Test Site near Socorro, New Mexico, on 14 September 1998.[2]

It has oneminor-planet moon, discovered in September 2003. It has anorbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters.[1][3] It is one ofseven known Aten binaries as of 2017.

Interaction with Earth

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1998 RO1's orbit is very eccentric, with anaphelion beyond the orbit ofMars and a perihelion inside the orbit ofMercury.[3] It has anorbital period of 360.29 days (0.99 years) and makes close approaches to Earth.[1] But1998 RO1 makes closer approaches to other inner planets, especially Mars. Its closest approach to a planet between 1950–2200 was to Mars, as it passed 0.00898 AU (1,343,000 km) from Mars on 18 March 1964, and will pass 0.0054 AU (810,000 km) from Mars on 12 October 2065.[1]

Moon

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Binary asteroid example

1998 RO1 has one unnamednatural satellite.[1] The satellite was discovered from lightcurve observations going from 13 to 28 September 2013, and was confirmed by radar observations from theArecibo Observatory one year later. It is in a very close orbit to1998 RO1, with a semi-major axis of 800 m (2,600 ft) and an eccentricity of 0.06,[3] giving it a periapsis of 752 m (2,467 ft) and an apoapsis of 848 m (2,782 ft). The satellite takes 14.54 hours to complete one orbit around1998 RO1.[3]

Numbering and naming

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Thisminor planet wasnumbered by theMinor Planet Center on 10 September 2003.[14] As of 2018, it has not beennamed.[2]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 66063 (1998 RO1)" (2010-09-10 last obs.).Jet Propulsion Laboratory. Retrieved18 November 2017.
  2. ^abc"66063 (1998 RO1)".Minor Planet Center. Retrieved18 November 2017.
  3. ^abcdefJohnston, Wm. Robert (20 September 2014)."Asteroids with Satellites Database – (66063) 1998 RO1".Johnston's Archive. Retrieved18 November 2017.
  4. ^abGalád, A.; Kornos, L.; Gajdos, S.; Világi, J.; Tóth, J. (October 2004). "Relative photometry of numbered asteroids (3712), (4197), (5587), (28753) and (66063)".Contributions of the Astronomical Observatory Skalnaté Pleso.34 (3): 157–166.(CoSkaHomepage).Bibcode:2004CoSka..34..157G.
  5. ^abPravec, P.; Kusnirak, P.; Sarounova, L.; Brown, P.; Esquerdo, G.; Pray, D.; et al. (October 2003). "(66063) 1998 RO_1".IAU Circ.8216 (8216): 3.Bibcode:2003IAUC.8216....3P.
  6. ^abScheirich, P.; Pravec, P. (April 2009). "Modeling of lightcurves of binary asteroids".Icarus.200 (2):531–547.Bibcode:2009Icar..200..531S.doi:10.1016/j.icarus.2008.12.001.
  7. ^abWolters, Stephen D.; Green, Simon F.; McBride, Neil; Davies, John K. (February 2008)."Thermal infrared and optical observations of four near-Earth asteroids"(PDF).Icarus.193 (2):535–552.Bibcode:2008Icar..193..535W.doi:10.1016/j.icarus.2007.08.011.
  8. ^"Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved18 November 2017.
  9. ^abcdPravec, P.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Mottola, S.; Hahn, G.; et al. (March 2006). "Photometric survey of binary near-Earth asteroids".Icarus.181 (1):63–93.Bibcode:2006Icar..181...63P.doi:10.1016/j.icarus.2005.10.014.
  10. ^abc"LCDB Data for (66063)". Asteroid Lightcurve Database (LCDB). Retrieved18 November 2017.
  11. ^Abell, P. A.; Gaffey, M. J.; Landis, R. R.; Jarvis, K. S. (March 2005). "Compositional Investigation of Binary Near-Earth Asteroid 66063 (1998 RO1): A Potentially Undifferentiated Assemblage".36th Annual Lunar and Planetary Science Conference: 2283.Bibcode:2005LPI....36.2283A.
  12. ^abCarry, 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.
  13. ^Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 February 2018.

External links

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