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(436724) 2011 UW158
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Stony, walnut-shaped asteroid and fast rotator
September 2020
yes
(436724) 2011 UW 158
#FFC2E0
2011UW158.jul14.p05us.p27Hz(1).gif
Animation of Arecibo radar images of 2011 UW 158 padding: 5px 0;
25 October 2011
Pan-STARRS 1
Haleakala Obs.
(436724) 2011 UW 158
ApolloNEOPHA
4 September 2017 (JD 2458000.5)
0
5.48 yr (2,003 days)
2.2301 AU
1.0109 AU
1.6205 AU
0.3762
2.06 yr (753 days)
12.072°
0.4778 ms / day
4.5717°
286.00°
8.7537°
0.0020 AU0.8 LD
0.22 0.04 km0.3 × 0.6 km0.311 km (calculated)
0.61069 0.00002 hlightcurve-plot0.61070 0.00003 h0.61073 h0.610752 0.000001 h
0.20 (assumed)0.39 0.09
S
19.45 0.2719.919.93 0.11
(436724) 2011 UW 158 is a stony, walnut-shaped asteroid and fast rotator, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 300 meters in diameter. It was discovered on 25 October 2011, by Pan-STARRS at Haleakala Observatory on the island of Maui, Hawaii, in the United States.
Orbital description
2011 UW 158 orbits the Sun at a distance of 1.0–2.2 AU once every 2 years and 1 month (753 days). Its orbit has an eccentricity of 0.38 and an inclination of 5° with respect to the ecliptic. Its observation arc begins with its official discovery observation by Pan-STARRS, as no precoveries were taken, and no prior identifications were made.
Close approach
The asteroid has an Earth minimum orbit intersection distance of 0.0020 AU km on off 2, which corresponds to 0.8 lunar distances (LD). On 19 July 2015, it passed about 2.5 million kilometers from Earth (6.5 LD), attracting the interest of astronomers. The asteroid was listed as level 1 in the Torino Scale on 4 November 2011, 9 days after its discovery, but was removed two weeks later.
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2011 UW158 July2015 flyby-orbits.png
2011 UW158 July2015 flyby-sky_trajectory.png
Left: Inner solar system orbits; right: Motion of 2011 UW 158 across sky, 6 hour motion
left
Physical characteristics
Spectral type
2011 UW 158 is an assumed stony S-type asteroid, the most common type among the populations of near-Earth and inner main-belt asteroids.
Diameter and albedo
Bruce Gary at Hereford Arizona Observatory (G95) estimated a mean diameter of 220 meters with a high albedo of 0.39, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroid of 0.20 and calculates a mean-diameter of 311 meters based on an absolute magnitude of 19.9.
Fast rotator
In July and August 2015, rotational lightcurves of this asteroid were obtained from photometric observations by Bruce Gary at Hereford Arizona Observatory and by Brian Warner at the CS3–Palmer Divide Station in California (U82). Lightcurve analysis gave a rotation period of 0.6107 hours (36.6 minutes) with a brightness variation between 0.52 and 2.05 magnitude (U=3/3/3).lightcurve-plot This makes 2011 UW 158 one of the top 200 fast rotators, suggesting it is a large boulder rather than a rubble pile.
Shape
Radar observations by the Arecibo Observatory on 14 July 2015, revealed that the asteroid's shape looks like an unshelled walnut with a diameter of 300 by 600 metres. The radiometric observations also agreed with the previously
obtained photometric ones and gave a period of 37 minutes.
Media attention
It also attracted the media and even firms such as Planetary ResourcesMining Firm Aiming For Platinum-Loaded Asteroid http://news.sky.com/story/1521488/mining-firm-aiming-for-platinum-loaded-asteroid https://web.archive.org/web/20150721185839/http://news.sky.com/story/1521488/mining-firm-aiming-for-platinum-loaded-asteroid dead 21 July 2015 2015-07-23 for its alleged content of platinum worth as high as 5 trillion U.S. dollars.UW-158: Watch live as asteroid worth £ 3 TRILLION passes close to Earth https://www.mirror.co.uk/news/world-news/uw-158-watch-live-asteroid-worth-6097254 2015-07-23https://metro.co.uk/2015/07/19/what-you-can-expect-to-see-as-a-3-trillion-asteroid-passes-earth-tonight-5302804/ What you can expect to see as a £3 trillion asteroid passes Earth tonight 2015-07-23http://main.slooh.com/event/5-trillion-dollar-asteroid-makes-close-approach-to-earth/ $5 Trillion Dollar Asteroid Makes Close Approach to Earth 2015-07-23 Commenters at StackExchange have denied these estimations as being "orders of magnitude too high",https://space.stackexchange.com/q/10048 How is it known that asteroid 2011 UW 158 has so much platinum? 2015-07-23 and radar observations have shown that the object contains no more metal than an average rocky asteroid.http://iaaweb.org/iaa/Scientific%20Activity/draftprogpdc17.pdf 5th IAA Planetary Defense Conference 2017-06-03 19 August 2019 https://web.archive.org/web/20190819120554/http://iaaweb.org/iaa/Scientific%20Activity/draftprogpdc17.pdf deadhttps://twitter.com/astrotweeps/status/865105034459189248 Ground-based radar observations of human space flight accessible targets 2017-06-03
Notes
lightcurve-plot Lightcurve plot of 2011 UW 158 by Brian Warner at the CS3–Palmer Divide Station in July 2015: rotation period of 0.61069 0.00002 hours with an amplitude of 0.65 magnitude
References
30em 2017-04-19 last obs.
JPL Small-Body Database Browser: 436724 (2011 UW158)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2436724
Jet Propulsion Laboratory
2 June 2017
436724 (2011 UW158)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=436724
28 March 2017
Solar System Studies at Arecibo Observatory
http://www.naic.edu/~pradar/news.php#2015
Arecibo Observatory
2015-07-23
2011 UW158 Impact Risk
Near Earth Object Program
NASA
http://neo.jpl.nasa.gov/risk/2011uw158.html
dead
https://web.archive.org/web/20111106205050/http://neo.jpl.nasa.gov/risk/2011uw158.html
November 6, 2011
NEOs Removed from Impact Risks Tables
Near Earth Object Program
NASA
http://neo.jpl.nasa.gov/risk/removed.html
https://web.archive.org/web/20020602101400/http://neo.jpl.nasa.gov/risk/removed.html
dead
2 June 2002
28 March 2017
First detailed images of rare asteroid to pass close by Earth on 19 July
19 July 2015
Astronomy Now
https://astronomynow.com/2015/07/19/first-detailed-images-of-rare-asteroid-to-pass-close-by-earth-on-19-july/
28 March 2017
436724
28 March 2017
Gary, Bruce L.
January 2016
Unusual Properties for the NEA (436724) 2011 UW158
https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016MPBu...43...33G
The Minor Planet Bulletin
43
1
33–38
1052-8091
2016MPBu...43...33G
28 March 2017
Warner, Brian D.
January 2016
Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2015 June–September
https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016MPBu...43...66W
The Minor Planet Bulletin
43
1
66–79
32455369
7244002
1052-8091
2016MPBu...43...66W
28 March 2017
Albino Carbognani
Bruce L. Gary
Julian Oey
Giorgio Baj
Paolo Bacci
January 2016
Pole and Shape for the NEA (436724) 2011 UW158
https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016MPBu...43...38C
The Minor Planet Bulletin
43
1
38–41
1052-8091
2016MPBu...43...38C
28 March 2017
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
November 2015
Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results
https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V
Icarus
261
34–47
2015Icar..261...34V
10.1016/j.icarus.2015.08.007
1506.00762
53493339 28 March 2017
External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
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