(4953) 1990 MU

Description

was first observed over three nights in 1990. By itself, this was not enough for the asteroid to be given a permanent number since the orbit could not be calculated accurately enough for the object to be subsequently recovered. However, the object was precovered by the Anglo-Australian Near-Earth Asteroid Survey on six photographic plates from the UK Schmidt Telescope dating back to 1974. This technique has more success with the Amor group of asteroids which do not cross the orbit of the Earth and consequently have long periods of opposition when they can be observed. In this respect the Apollo asteroid is somewhat unusual.

has an Earth minimum orbit intersection distance (MOID) of 0.0263 AU, which is close enough to classify it as a potentially hazardous asteroid (PHA). It will make a close approach to Earth on 6 June 2027 at 0.0308 AU, and even closer on 5 June 2058 at 0.0231 AU. It also made a close approach to Venus on 5 October 2012 at 0.0567 AU and will again on 3 September 2041 at 0.0581 AU. The Earth MOID of has been decreasing (becoming more hazardous) during the 20th century, while the Venus MOID (0.0455) has been increasing.

Besides its original discovery at Siding Spring Observatory in Australia, has also been studied by radar at Goldstone Observatory in California, and Arecibo Observatory in Puerto Rico. Lightcurves have been obtained at La Silla Observatory in Chile.

The albedo of was measured by the ExploreNEOs project of the Spitzer Space Telescope in August 2009. The result obtained was 0.79 and was the second highest albedo measured by the project. However, ExploreNEO do not believe this is a plausible figure, they state that the albedo of an NEO is not likely to be much over 0.5 and their measurement uncertainty is "around a factor of 2".

The Gaia mission of the European Space Agency, launched in December 2013, has been tasked with measuring the Yarkovsky effect on near-Earth asteroids (NEAs). The Yarkovsky effect is a small non-gravitational force on rotating bodies that can affect their trajectories. Its effect on small bodies like asteroids can be significant and needs to be taken into account in predicting an asteroid's position. has been selected as one of the most promising NEAs for this measurement by Gaia.

References

|archive-url= https://web.archive.org/web/20171107024450/http://earn.dlr.de/nea/004953.htm |archive-date=7 November 2017 |url-status=dead

References

1. (1994). "Hazards Due to Comets and Asteroids". [[University of Arizona Press]].
2. (1992). "Anglo-Australian Near-Earth Asteroid Survey". Liège International Astrophysical Colloquia.
3. (1995). "Near-Earth Asteroids on Archival Schmidt Plates". IAU Colloquium 148: The Future Utilisation of Schmidt Telescopes.
4. "AstDys 2003AZ84 Ephemerides". Department of Mathematics, University of Pisa, Italy.
5. (1994). "Hazards Due to Comets and Asteroids". [[University of Arizona Press]].
6. (June 1994). "Asteroid Radar Astronomy at Goldstone in the 1990s".
7. (2004). "Mitigation of Hazardous Comets and Asteroids". [[Cambridge University Press]].
8. (1993). "Differential CCD Photometry of 1980 Tezcatlipoca, 2368 Beltrovata 4769 Castalia, 4953 1990 MU and 4954 Eric". [[Lunar and Planetary Institute]].
9. (September 1, 2010). "ExploreNEOs. I. Description and First Results from the Warm Spitzer Near-Earth Object Survey". [[The Astronomical Journal]].
10. Bergin, Chris. (December 19, 2013). "Soyuz ST-B successfully launches Gaia space observatory".
11. (2011). "Detecting the Yarkovsky effect with the Gaia mission: List of the most promising candidates". Monthly Notices of the Royal Astronomical Society.
12. "JPL Small-Body Database Search Engine".
13. [https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=16960;old=0;orb=0;cov=0;log=0;cad=1#cad JPL Small-Body Database Browser: 16960 (1998 QS52)]
14. [https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=89830;old=0;orb=0;cov=0;log=0;cad=1#cad JPL Small-Body Database Browser: 89830 (2002 CE)]
15. [https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4183;old=0;orb=0;cov=0;log=0;cad=1#cad JPL Small-Body Database Browser: 4183 Cuno (1959 LM)]
16. "JPL Small-Body Database Browser: 3200 Phaethon (1983 TB)".
17. "JPL Small-Body Database Browser: 4953 (1990 MU)".
18. "JPL Small-Body Database Browser: 4953 (1990 MU)". [[Jet Propulsion Laboratory]].