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(162421) 2000 ET70
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Near-Earth asteroid
October 2019
yes
(162421) 2000 ET 70
#FFC2E0
LINEAR
Lincoln Lab's ETS
8 March 2000
(162421) 2000 ET 70
NEOPHAAten
4 September 2017 (JD 2458000.5)
0
37.17 yr (13,575 d)
1.0638 AU
0.8295 AU
0.9467 AU
0.1237
0.92 yr (336 days)
129.36°
1.0701 ms / day
22.323°
331.16°
46.103°
0.0316 AU12.3 LD
2.6×2.2×2.1 km2.9×2.2×1.5 km2.0 0.2 km2.10 0.07 km2.26 0.11 km
8.94 0.04 h8.9444 0.0008 h8.947 0.001 hlightcurve-plot-Oey8.96 0.01 h
0.018 0.0020.065 0.05
Xk
18.018.2
(162421) 2000 ET 70 is a dark, elongated and oblate asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group, approximately 2.2 kilometers in diameter. It was discovered on 8 March 2000, by astronomers of the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico. The body has a notably low albedo, and its shape resembles that of a "clenched fist".
Orbit and classification
2000 ET 70 orbits the Sun at a distance of 0.8–1.1 AU once every 11 months (336 days; semi-major axis of 0.95 AU). Its orbit has an eccentricity of 0.12 and an inclination of 22° with respect to the ecliptic. A first precovery was found in the Digitized Sky Survey from images taken at ESO's La Silla Observatory in February 1977. The body's observation arc begins with its official discovery observation at Socorro in March 2000.
Close approaches
The asteroid has an Earth minimum orbital intersection distance of 0.0316 AU km on off 3 which translates into 12.3 lunar distances. In February 2012, it was observed by radar during a close approach (0.045 AU) at the Arecibo and Goldstone observatories. The observations allowed to model the body's spin period and rotation, as well as its shape (see below).
Physical characteristics
2000 ET 70 has been characterized as a Xk-subtype, which transitions between the X- and K-type asteroids.
Rotation period, pole, and shape
During its close approach in February 2012, a rotational lightcurve of 2000 ET 70 was obtained from photometric observations by a collaboration of astronomers from Uruguay, Australia, and the United States. Analysis of the lightcurve gave a period of 8.947 hours with a brightness amplitude of 0.60 magnitude (U=3-).lightcurve-plot-Oey
Radar observations at Arecibo and Goldstone showed that the asteroid spins in a retrograde manner with a rotation period of 8.96 hours. It is likely a principal axis rotator, i.e., not tumbling. Shape modelling by two independent teams gave sidereal periods of 8.96 and 8.944 hours, respectively. A spin axis of (80.0°, −50.0°) in ecliptic coordinates was determined. The observations also revealed that the asteroid has an elongated oblate shape, resembling a "clenched fist". Its surface exhibits multiple kilometer scale ridges and concavities.
Diameter and albedo
According to shape modeling of radar observations, the asteroid's overall dimensions are 2.6×2.2×2.1 kilometers. Based on an absolute magnitude of 18.2, this results in a notably low albedo of 0.018. More recent modeling combining radar, photometric, and infrared data gave and even more elongated shape of 2.9×2.2×1.5 kilometers. These authors argue that the absolute magnitude value is incorrect and report a geometric albedo of 0.09.
2000 ET 70's mean-diameter measures between 2.0 and 2.26 kilometers and its surface has an albedo between 0.018 and 0.09. The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.018 and a diameter of 2.26 kilometers based on an absolute magnitude of 18.2.
Numbering and naming
This minor planet was numbered on 26 September 2007, after its orbital parameters had been sufficiently determined (M.P.C. 60670). As of 2018, it has not been named.
Notes
lightcurve-plot-Oey Lightcurve plot of (162421) 2000 ET 70, by Julian Oey (2012) at Blue Mountains Observatory (Kingsgrove Observatory; E19). Lightcurve period 8.970 0.004 hours. Note: additional photometric data from other observatories gave a refined period of 8.947 hours. Summary figures at the LCDB
References
30em 2014-04-20 last obs.
JPL Small-Body Database Browser: 162421 (2000 ET70)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2162421
Jet Propulsion Laboratory
28 November 2017
162421 (2000 ET70)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=162421
28 November 2017
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
28 November 2017
162421
28 November 2017
6
Shantanu Naidu
J. L. Margot
P. A. Taylor
M. C. Nolan
M. Brozovic
L. A. M. Benner
J. D. Giorgini
E. S. Howell Ellen Howell
M. W. Busch
C. Magri
October 2012
Radar Observations and Shape Modeling of Near-Earth Asteroid (162421) 2000 ET70
American Astronomical Society
302.06 2012DPS....4430206N
6
Shantanu P. Naidu
Jean-Luc Margot
Michael W. Busch
Patrick A. Taylor
Michael C. Nolan
Marina Brozovic
Lance A. M. Benner
Jon D. Giorgini
Christopher Magri
September 2013
Radar imaging and physical characterization of near-Earth Asteroid (162421) 2000 ET70
Icarus
226
1
323–335
2013Icar..226..323N
10.1016/j.icarus.2013.05.025
1301.6655
6
Sean E. Marshall
Ellen S. Howell Ellen Howell
Christopher Magri
Ronald J. Vervack
Donald B. Campbell
Yanga R. Fernández
Michael C. Nolan
Jenna L. Crowell
Michael D. Hicks
Kenneth J. Lawrence
Patrick A. Taylor
August 2017
Thermal properties and an improved shape model for near-Earth asteroid (162421) 2000 ET70
Icarus
292
22–35
2017Icar..292...22M
10.1016/j.icarus.2017.03.028
1610.04653
6
Eduardo Manuel Alvarez
Julian Oey
Xianming L. Han
Orry R. Heffner
Adam W. Kidd
Bradley J. Magnetta
Frederick W. Rastede
July 2012
Period Determination for NEA (162421) 2000 ET70
The Minor Planet Bulletin
39
3
170
1052-8091
2012MPBu...39..170A
External links
Imaging near-Earth asteroid (162421) 2000 ET70
Asteroid (162421) 2000 ET70 3D model
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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