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2018 CB

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2018 CB
Highly elliptical orbit of2018 CB,crossing those of both Mars and Earth. Positions shown for 1 January 2018, before flyby.
Discovery[1]
Discovered byCSS
Discovery siteMount Lemmon Obs.
Discovery date4 February 2018
(first observed only)
Designations
2018 CB
NEO·Apollo[1][2]
Earth-andMars crosser
Orbital characteristics[2]
Epoch23 March 2018 (JD2458200.5)
Uncertainty parameter2
Observation arc5 days
Aphelion1.8589AU
Perihelion0.9582 AU
1.4085 AU
Eccentricity0.3197
1.67yr(611 days)
10.249°
0° 35m22.56s/ day
Inclination5.3027°
320.79°
208.11°
EarthMOID0.0004 AU (0.2LD)
Physical characteristics
7m(assumed)[3]
20 m(upper limit)
>0.18
~1(assumed)[3]
26.0[2]

2018 CBis a very bright micro-asteroid,classified as anear-Earth objectof theApollo group,less than 20 meters (66 ft) in diameter. It was first observed by astronomers of theCatalina Sky SurveyatMount Lemmon Observatory,Arizona, on 4 February 2018, during its sub-lunar close encounter with Earth.[1]

2018 flyby

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On 9 February 2018, the asteroid passed about 64,500 km (40,100 mi) from Earth, traveling 10 miles per second (16 km/s) relative to Earth and briefly reachingapparent magnitude13.[4]It was observed by theGoldstone Observatory,which constrained its size to no more than 20 meters.[3]

During the flyby its period was changed from 1.48 years to 1.67 years.[2]

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  • Its path across the sky on February 9 was north to south (30 minute positions shown)
    Its path across the sky on February 9 was north to south (30 minute positions shown)
  • Seen from space, it passes just outside geosynchronous orbit
    Seen from space, it passes just outside geosynchronous orbit
  • 20 minute timelapse, taken two days before closest approach. The asteroid can be seen near the center of the image, moving towards the lower left. Brightness is inverted (stars appear dark, the sky background appears light).[5]
    20 minute timelapse, taken two days before closest approach. The asteroid can be seen near the center of the image, moving towards the lower left. Brightness is inverted (stars appear dark, the sky background appears light).[5]
  • 2018 CB on February 7. The image is corrected for the asteroid's motion, so stars appear trailed.[6]
    2018 CB on February 7. The image is corrected for the asteroid's motion, so stars appear trailed.[6]

Other flybys

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2018 CB's orbit is in Earth's neighborhood, so it frequently makes other close approaches to Earth like the 2018 one, although not usually as close. In 1953 (65 years or 44 orbits earlier), it passed 0.00650 AU (972,000 km; 604,000 mi) from Earth, and in 2090 it will pass between 0.00475 AU (711,000 km; 442,000 mi) and 0.00798 AU (1,194,000 km; 742,000 mi) from Earth.

It also may have passed similarly near Earth in 1914, but the uncertainty in the 1953 approach makes it difficult to determine.

Physical characteristics

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2018 CBappears unusually bright for its size, suggesting it is made of brighter materials than the average asteroid.

See also

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References

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  1. ^abc"2018 CB".Minor Planet Center.Retrieved15 February2018.
  2. ^abcd"JPL Small-Body Database Browser: (2018 CB)"(2018-02-09 last obs.).Jet Propulsion Laboratory.Retrieved15 February2018.
  3. ^abcBenner, Lance."2018 CB Astrometry - Minor Planet Mailing List".groups.yahoo.Retrieved9 February2018.
  4. ^Bob King (5 February 2018)."Asteroids 2018 CB And CC Graze Earth This Week — Watch It Online".Astro Bob.
  5. ^Wells, G.; Bamberger, D. (8 February 2018)."Very close approacher 2018 CB (Video)".Northolt Branch Observatories, Facebook.Retrieved11 February2018.
  6. ^Wells, G.; Bamberger, D. (8 February 2018)."Very close approacher 2018 CB".Northolt Branch Observatories, Facebook.Retrieved11 February2018.
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