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(66063) 1998 RO1
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Stony near-Earth object of the Aten group
October 2019
yes
(66063) 1998 RO 1
#FFC2E0
Orbit of (66063) 1998 RO1.gif
Orbit of 1998 RO 1
LINEAR
Lincoln Lab's ETS
14 September 1998
(66063) 1998 RO 1
1999 SN 5
NEOAten
4 September 2017 (JD 2458000.5)
0
13.99 yr (5,111 days)
1.7045 AU
0.2774 AU
0.9910 AU
0.7200
0.99 yr (360 days)
348.97°
0.9991 ms / day
22.678°
351.88°
151.13°
0.0921 AU35.9 LD
1 (D: 0.38 km; P: 14.53 h)
0.62 0.25 km0.72 km (est. at 0.20)0.8 0.15 km0.860 km (derived)
2.8 1.3 g/cm3
2.4924 0.0003 h2.4924 h
0.1450.30 0.17
S
18.0018.0418.0518.05 0.07118.1
(66063) 1998 RO 1 is a stony near-Earth object of the Aten group on a highly-eccentric orbit. The synchronous binary system measures approximately 800 m mi off us in diameter. It was discovered by astronomers of the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, on 14 September 1998.
It has one minor-planet moon, discovered in September 2003. It has an orbital period of 14.53 hours and measures approximately 48% of its primary, or 380 meters. It is one of seven known Aten binaries as of 2017.
Interaction with Earth
1998 RO 1's orbit is very eccentric, with an aphelion beyond the orbit of Mars and a perihelion inside the orbit of Mercury. It has an orbital period of 360.29 days (0.99 years) and makes close approaches to Earth. But 1998 RO 1 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 km on from Mars on 18 March 1964, and will pass 0.0054 AU km on from Mars on 12 October 2065.
Moon
thumb|left|100px|Binary asteroid example
1998 RO 1 has one unnamed natural satellite. The satellite was discovered from lightcurve observations going from 13 to 28 September 2013, and was confirmed by radar observations from the Arecibo Observatory one year later. It is in a very close orbit to 1998 RO 1, with a semi-major axis of 800 m ft on and an eccentricity of 0.06, giving it a periapsis of 752 m ft on and an apoapsis of 848 m ft on. The satellite takes 14.54 hours to complete one orbit around 1998 RO 1.
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 10 September 2003. As of 2018, it has not been named.
References
2010-09-10 last obs.
JPL Small-Body Database Browser: 66063 (1998 RO1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2066063
Jet Propulsion Laboratory
18 November 2017
66063 (1998 RO1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=66063
18 November 2017
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
24 February 2018
Asteroids with Satellites Database – (66063) 1998 RO1
Johnston's Archive
20 September 2014
Johnston, Wm. Robert
http://www.johnstonsarchive.net/astro/astmoons/am-66063.html
18 November 2017
Asteroid Size Estimator
CNEOS NASA/JPL
https://cneos.jpl.nasa.gov/tools/ast_size_est.html
18 November 2017
66063
18 November 2017
Stephen D. Wolters
Simon F. Green
Neil McBride
John K. Davies
February 2008
Thermal infrared and optical observations of four near-Earth asteroids
Icarus
193
2
535–552
2008Icar..193..535W
10.1016/j.icarus.2007.08.011 http://oro.open.ac.uk/10790/2/10790.pdf
6
P. Pravec
P. Kusnirak
L. Sarounova
P. Brown
G. Esquerdo
D. Pray
L. A. M. Benner
M. C. Nolan
J. D. Giorgini
S. J. Ostro
J.-L. Margot
October 2003
(66063) 1998 RO_1
IAU Circ.
8216 3 2003IAUC.8216....3P
A. Galád
L. Kornos
S. Gajdos
J. Világi
J. Tóth
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)
2004CoSka..34..157G
6
P. Pravec
P. Scheirich
P. Kusnirák
L. Sarounová
S. Mottola
G. Hahn
P. Brown
G. Esquerdo
N. Kaiser
Z. Krzeminski
D. P. Pray
B. D. Warner
A. W. Harris
M. C. Nolan
E. S. Howell
L. A. M. Benner
J.-L. Margot
A. Galád
W. Holliday
M. D. Hicks
Yu. N. Krugly
D. Tholen
R. Whiteley
F. Marchis
D. R. DeGraff
A. Grauer
S. Larson
F. P. Velichko
W. R. Cooney
R. Stephens
J. Zhu
K. Kirsch
R. Dyvig
L. Snyder
V. Reddy
S. Moore
S. Gajdos
J. Világi
G. Masi
D. Higgins
G. Funkhouser
B. Knight
S. Slivan
R. Behrend
M. Grenon
G. Burki
R. Roy
C. Demeautis
D. Matter
N. Waelchli
Y. Revaz
A. Klotz
M. Rieugné
P. Thierry
V. Cotrez
L. Brunetto
G. Kober
March 2006
Photometric survey of binary near-Earth asteroids
Icarus
181
1
63–93
2006Icar..181...63P
10.1016/j.icarus.2005.10.014
Petr Pravec
Alan W. Harris
Peter Kusnirák
Adrián Galád
Kamil Hornoch
September 2012
Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations
Icarus
221
1
365–387
2012Icar..221..365P
10.1016/j.icarus.2012.07.026 11104/0217021
free
B. Carry
E. Solano
S. Eggl
F. E. DeMeo
April 2016
Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry
Icarus
268
340–354
2016Icar..268..340C
10.1016/j.icarus.2015.12.047
1601.02087 119258489
P. Scheirich
P. Pravec
April 2009
Modeling of lightcurves of binary asteroids
Icarus
200
2
531–547
2009Icar..200..531S
10.1016/j.icarus.2008.12.001
P. A. Abell
M. J. Gaffey
R. R. Landis
K. S. Jarvis
March 2005
Compositional Investigation of Binary Near-Earth Asteroid 66063 (1998 RO1): A Potentially Undifferentiated Assemblage
36th Annual Lunar and Planetary Science Conference
2283
2005LPI....36.2283A
External links
Binary and Ternary Near-Earth Asteroids Detected by Radar, Lance Benner, JPL
Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
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