Английская Википедия:3122 Florence

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3122 Florence is a stony[1] trinary[2] asteroid of the Amor group. It is classified as a near-Earth object and potentially hazardous asteroid. It measures approximately 5 kilometers in diameter. It orbits the Sun at a distance of 1.0–2.5 AU once every 2 years and 4 months (859 days); the orbit has an eccentricity of 0.42 and an inclination of 22° with respect to the ecliptic.[3] Florence has two moons.

Florence was discovered on 2 March 1981 by American astronomer Schelte J. "Bobby" Bus at Siding Spring Observatory.[4] Its provisional designation was Шаблон:Mp. It was named in honor of Florence Nightingale, the founder of modern nursing;[5] the naming citation was published on 6 April 1993 (Шаблон:Small).[6]

Florence is classified as a potentially hazardous object because its minimum orbit intersection distance Шаблон:Nowrap indicates that it has the potential to make close approaches to the Earth, and because measurements of its absolute magnitude Шаблон:Nowrap suggest that it is large enough to create serious damage were it to impact.[3][7]

Moons

Файл:3122 Florence with moons.jpg
Trinary asteroid: Florence with its two satellites

Radar observations during the 2017 flyby have shown that Florence has two moons. The inner of the two moons is estimated to have a diameter of 180 to 240 meters, the outer moon is between 300 and 360 meters across. Each moon is somewhat elongated, and both are tidally locked to the main body. They probably formed as loose material spun away from the main body as its rotation accelerated due to the YORP effect.[1]

The inner moon's period orbiting Florence appears to be approximately 7 hours, while the outer moon completes a revolution in about 21 to 23 hours. The inner moon of Florence has the shortest orbital period of any of the moons of the 60 near-Earth asteroids known to have moons.[1]

Florence is only the third known trinary asteroid in the near-Earth asteroid population, after Шаблон:Mpl and Шаблон:Mpl.

2017 close approach

Шаблон:As of Шаблон:Convert from Earth, approximately eighteen times the average distance of the Moon.[8] As seen from Earth, it brightened to apparent magnitude 8.5, and was visible in small telescopes for several nights as it moved south to north through the constellations Piscis Austrinus, Capricornus, Aquarius, and Delphinus.[9] This was the asteroid's closest approach since 1890 and the closest until after 2500.[10][11][12] Its previous flyby was on 29 August 1930, at a distance of 0.05239 AU and the next one will be on 2 September 2057, at 0.049952 AU.[13]

Radar imagery

During the flyby, scientists studied Florence using the Arecibo Observatory and the Goldstone Deep Space Communications Complex, and discovered that it has two moons.[2][14]

Goldstone Radar
Arecibo Radar

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:2017 in space Шаблон:Authority control

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  7. Шаблон:Cite web
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  9. Шаблон:Cite news
  10. Шаблон:Cite news
  11. Шаблон:Cite web
  12. Шаблон:Cite web
  13. 13,0 13,1 Шаблон:Cite web
  14. 14,0 14,1 Шаблон:Cite web
  15. Шаблон:Cite web
  16. Шаблон:Cite web
  17. Шаблон:Cite web
  18. Шаблон:Cite web