164207 Cardea

Sub-kilometer asteroid and quasi-satellite of Earth From Wikipedia, the free encyclopedia

164207 Cardea (provisional designation 2004 GU9) is a sub-kilometer asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group. It is a quasi-satellite of Earth, a situation that should persist until around 2600, when it is expected to shift to a regular horseshoe orbit for a few thousand years.[4]

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164207 Cardea
Cardea photographed by the Canada–France–Hawaii Telescope in February 2007
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date13 April 2004
Designations
(164207) Cardea
Pronunciation/ˈkɑːrdiə/
Named after
Cardea
2004 GU9
NEO Â· Apollo
Orbital characteristics[2]
Epoch 21 November 2025 (JD 2461000.5)
Uncertainty parameter 0
Observation arc8688 days (23.79 yr)
Aphelion1.1372 AU (170.12 Gm)
Perihelion0.8650 AU (129.40 Gm)
1.0011 AU (149.76 Gm)
Eccentricity0.1359
1.0017 yr (365.87 d)
97.3298°
0° 59m 1.464s / day
Inclination13.6529°
38.3866°
280.55672±0.00007°
2456145.53817±0.00006 jd
279.3410°
Earth MOID0.0031 AU (460,000 km)
Physical characteristics
163 m[3]: 2988 
0.219[3]: 2988 
21.1[2]
Close

On 14 April 2004 (with less than a 1-day observation arc), the Sentry Risk Table showed 180 virtual impactors.[5] It was removed from the Sentry Risk Table 2 days later on 16 April 2004.[6] As later precovery observations by Haleakala-AMOS from 2001 have been found, Cardea now has a well determined orbit with an observation arc of 24 years.[1]

Discovery and naming

This asteroid was discovered on 13 April 2004 by the Lincoln Near-Earth Asteroid Research (LINEAR) project near Socorro, New Mexico and given the provisional designation 2004 GU9.[1] Following the naming of 524522 Zoozve, a quasi-satellite of Venus, Radiolab and the International Astronomical Union held a public naming campaign for this quasi-satellite from June to September 2024.[7][8] Seven finalist names were revealed in December 2024, with the names being Bakunawa, Cardea, Ehaema, Enkidu, Ótr, Tarriaksuk, and Tecciztecatl.[9] The winning name was Cardea, the Roman goddess of the hinge. The name was announced by the International Astronomical Union on 13 January 2025.[10]

Orbit

Cardea orbits the Sun with a semi-major axis of 1.001 astronomical units (AU), taking 365.87 days to complete one orbit. It is classified as a near-Earth asteroid (NEA) and an Apollo asteroid;[2] Apollo asteroids are NEAs that cross Earth's orbit but have semi-major axes above 1 AU.[11] Its orbit is inclined by 13.653° with respect to the ecliptic plane. Along its orbit, its distance from the Sun varies from 0.865 AU at perihelion to 1.137 AU at aphelion due to its moderate[3]: 2987  orbital eccentricity of 0.136.[2]

Cardea is in a 1:1 mean-motion resonance with Earth, and it currently orbits in a quasi-satellite configuration.[4]: 489  Quasi-satellites have principal libration angles [a] that librate around 0°,[4]: 488  appearing to distantly orbit Earth from its perspective despite directly orbiting the Sun. All Earth quasi-satellites are temporary;[12] Cardea has been a quasi-satellite for about 600 years, and will eventually lose its status as one in about 500 years. Perturbations from Venus play a role in destabilizing Cardea from its quasi-satellite configuration even though their orbits do not cross. Currently, the libration of Cardea's has an amplitude of 8–10°, with a libration period of 70 years. After exiting its quasi-satellite phase, it will enter a horseshoe configuration.[4]: 490–491 

Physical characteristics

Cardea has a diameter of 163 metres (535 ft) and an albedo of 0.219.[3]: 2988 

Animation of 164207 Cardea's orbit from 1600 to 2500
Relative to Sun and Earth
Around Earth
Around Sun
   Sun Â·    Earth Â·   Cardea

See also

Notes

  1. Where and are the mean longitudes of Cardea and Earth, respectively

References

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