2007 WD5

2007 WD5
Discovery
Discovered by Andrea Boattini
Discovery date November 20, 2007
Designations
none
Apollo asteroid,[1]
Mars-crosser asteroid
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 5
Aphelion 3.9289 AU (587.76 Gm)
Perihelion 0.991120 AU (148.2694 Gm)
2.4600 AU (368.01 Gm)
Eccentricity 0.59711
3.86 yr (1409.3 d)
12.5 km/s (27,900 mph)[2]
49.267°
Inclination 2.4276°
68.491°
309.622°
Earth MOID 0.0260299 AU (3.89402 Gm)
Jupiter MOID 1.52869 AU (228.689 Gm)
Physical characteristics
Dimensions 50 m (160 ft)[3]H
24.3

    2007 WD5 is an Apollo asteroid some 50 m (160 ft) in diameter[1] and a Mars-crosser asteroid discovered on November 20, 2007, by Andrea Boattini of the Catalina Sky Survey. Early observations of 2007 WD5 caused excitement amongst the scientific community when it was estimated as having as high as a 1 in 25 chance of colliding with Mars on January 30, 2008.[4] However, by January 9, 2008, additional observations allowed NASA's Near Earth Object Program (NEOP) to reduce the uncertainty region resulting in only a 1-in-10,000 chance of impact.[5] 2007 WD5 most likely passed Mars at a distance of 6.5 Mars radii. Due to this relatively small distance and the uncertainty level of the prior observations, the gravitational effects of Mars on its trajectory are unknown and, according to Steven Chesley of NASA's Jet Propulsion Laboratory Near-Earth Object program, 2007 WD5 is currently considered 'lost' (see lost asteroids).[6]

    Discovery

    The asteroid was discovered on November 20, 2007 by Andrea Boattini[7] of the NASA-funded Catalina Sky Survey on Mount Lemmon, near Tucson, Arizona, USA, using a 1.5-meter telescope.[3] It was discovered in the constellation Taurus at an apparent magnitude of +20. This is about 400,000 times fainter than most people can see with the naked eye on a dark night far from city lights.[7] It was discovered nineteen days after passing near the Earth. By the time it arrived at Mars it had an apparent magnitude of roughly +26 and therefore appeared over 100x fainter than at the time of discovery.[8]

    Mars encounter: chance of impact

    Timeline of observations and events

    This trend of increasing probability of impact followed by a dramatic decrease is typical as uncertainties are gradually reduced.[5] In December 2004, a similar trend was observed with 99942 Apophis where the predicted probability of impact with Earth in 2029 at one point reached as high as 2.7%.

    NASA Animation showing the motion of the uncertainty region of 2007 WD5 as it approaches Mars. The thin white line is the orbit of Mars. The blue line traces the motion of the center of the uncertainty region, which is the most likely position of the asteroid. Orbital data as known on December 21, 2007

    Estimates of resulting impact

    Track of asteroid 2007 WD5 over Mars (NASA/JPL)

    If the asteroid had collided with Mars, it would have hit with a velocity of about 13.5 km/s (8.4 miles per second), and would have produced an explosion equivalent to about 3 megatons of TNT.[3] Due to the thin atmosphere of Mars, it was predicted that the asteroid would have reached the surface intact and blasted out a crater approximately 0.8 km (0.5 mi) in diameter.[13] A crater this size would be equal to the size of the Meteor Crater in Arizona, USA. NASA officials say if it had hit Mars, it would have done so north of the location of the Opportunity rover.[7]

    2007 WD5 is roughly the size of the cometary object that caused the Tunguska event in 1908, in remote central Siberia, Russia. Due to the Earth's greater gravity, an impact with the power of Tunguska is expected to occur once every few hundred years.[14] Since Mars has only 1/10 the mass to attract objects, these types of impacts occur roughly every one thousand years on Mars.[2]

    Future encounters

    In July 2003, the asteroid passed within 0.012 AU of Mars.[12] The exact fate of 2007 WD5 following the January 2008 Mars encounter is unknown although it likely passed Mars at a distance of 6.5 Mars radii. Mars, unlike Jupiter, is not big enough to eject the asteroid from the Solar System, however, the gravitation effect from the encounter on the asteroid's trajectory is uncertain and the asteroid is currently considered 'lost'.[6] Assuming 2007 WD5 passed Mars safely, its low inclination to the ecliptic of only 2.3 degrees and high eccentricity of 0.6 could cause it to swing close to Mars or Earth for years or decades into the future.

    See also

    References

    1. 1 2 3 "JPL Small-Body Database Browser: 2007WD5". Retrieved 30 March 2016.
    2. 1 2 "Astronomers Monitor Asteroid to Pass Near Mars". NASA/JPL. 2007-12-21. Archived from the original on 24 December 2007. Retrieved 2007-12-22.
    3. 1 2 3 4 5 Steve Chesley & Paul Chodas (December 21, 2007). "Recently Discovered Asteroid Could Hit Mars in January". NASA/JPL Near-Earth Object Program Office. Archived from the original on 24 December 2007. Retrieved 2007-12-21.
    4. 1 2 Don Yeomans; Paul Chodas & Steve Chesley (December 28, 2007). "Mars Impact Probability Increases to 4 Percent". NASA/JPL Near-Earth Object Program Office. Archived from the original on 29 December 2007. Retrieved 2007-12-28.
    5. 1 2 3 Steve Chesley; Paul Chodas & Don Yeomans (January 9, 2008). "2007 WD5 Mars Collision Effectively Ruled Out - Impact Odds now 1 in 10,000". NASA/JPL Near-Earth Object Program Office. Archived from the original on 11 January 2008. Retrieved 2008-01-09.
    6. 1 2 Lakdawalla, Emily (February 4, 2008). "WD5 most likely missed Mars, but we may never know". Archived from the original on 8 February 2008. Retrieved 2008-02-24.
    7. 1 2 3 4 Lori Stiles, University Communications (December 21, 2007). "Catalina Sky Survey Discovers Space Rock That Could Hit Mars". The University of Arizona. Retrieved 2007-12-23.
    8. ↑ Horizons Brightness Difference between 11-20-07 and 01-30-08: (5th root of 100) ^ (@marsJan30th APmag 25.9 - DiscoveryNov20th APmag 20.2) = 190x
    9. ↑ "Horizons Archive Mars/Earth 2003/2008". Retrieved 2007-12-23. (Soln.date: 2007-Dec-23)
    10. ↑ Don Yeomans; Paul Chodas & Steve Chesley (January 2, 2008). "New Observations Slightly Decrease Mars Impact Probability". NASA/JPL Near-Earth Object Program Office. Archived from the original on 5 January 2008. Retrieved 2008-01-02.
    11. ↑ Steve Chesley; Paul Chodas & Don Yeomans (January 8, 2008). "Mars Impact Seems Less Likely". NASA/JPL Near-Earth Object Program Office. Archived from the original on 12 January 2008. Retrieved 2008-01-08.
    12. 1 2 "Horizons Output Mars/Earth 2003/2008". Retrieved 2008-01-09. (Soln.date: 2008-Jan-09)
    13. ↑ Johnson Jr., John (2007-12-21). "Asteroid on track for possible Mars hit". Science (Los Angeles Times). Archived from the original on 22 December 2007. Retrieved 2007-12-21.
    14. ↑ David Morrison (2007-12-21). "Tunguska Revision, and a Possible NEA Impact on Mars". Asteroid and Comet Impact Hazards (NASA). Archived from the original on 2 January 2008. Retrieved 2008-01-03.

    External links

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