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2018 CB

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2018 CB
Highly elliptical orbit of 2018 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- and Mars crosser
Orbital characteristics [2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 2
Observation arc5 days
Aphelion1.8589 AU
Perihelion0.9582 AU
1.4085 AU
Eccentricity0.3197
1.67 yr (611 days)
10.249°
0° 35m 22.56s / day
Inclination5.3027°
320.79°
208.11°
Earth MOID0.0004 AU (0.2 LD)
Physical characteristics
7 m (assumed)[3]
20 m (upper limit)
>0.18
~1 (assumed)[3]
26.0[2]

2018 CB is a very bright micro-asteroid, classified as a near-Earth object of the Apollo group, less than 20 meters (66 ft) in diameter. It was first observed by astronomers of the Catalina Sky Survey at Mount Lemmon Observatory, Arizona, on 4 February 2018, during its sub-lunar close encounter with Earth.[1]

2018 flyby

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 reaching apparent magnitude 13.[4] It was observed by the Goldstone 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]

  • Its path across the sky on February 9th was north to south (30 minute positions shown)
    Its path across the sky on February 9th 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 7th. The image is corrected for the asteroid's motion, so stars appear trailed.[6]
    2018 CB on February 7th. The image is corrected for the asteroid's motion, so stars appear trailed.[6]

Other flybys

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

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

See also

References

  1. ^ a b c "2018 CB". Minor Planet Center. Retrieved 15 February 2018.
  2. ^ a b c d "JPL Small-Body Database Browser: (2018 CB)" (2018-02-09 last obs.). Jet Propulsion Laboratory. Retrieved 15 February 2018.
  3. ^ a b c Benner, Lance. "2018 CB Astrometry - Minor Planet Mailing List". groups.yahoo.com. Retrieved 9 February 2018.
  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. Retrieved 11 February 2018.
  6. ^ Wells, G.; Bamberger, D. (8 February 2018). "Very close approacher 2018 CB". Northolt Branch Observatories, Facebook. Retrieved 11 February 2018.
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