Английская Википедия:1620 Geographos

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1620 Geographos (Шаблон:IPAc-en), provisional designation Шаблон:Mp, is a highly elongated, stony asteroid, near-Earth object and potentially hazardous asteroid of the Apollo group, with a mean-diameter of approximately Шаблон:Convert. It was discovered on 14 September 1951, by astronomers Albert George Wilson and Rudolph Minkowski at the Palomar Observatory in California, United States.[1] The asteroid was named in honor of the National Geographic Society.[2]

Orbit and classification

Файл:Animation of 1620 Geographos orbit.gif
Animation of 1620 GeographosШаблон:'s orbit 2010-2020
Шаблон:Legend2Шаблон:·Шаблон:Legend2Шаблон:·Шаблон:Legend2Шаблон:·Шаблон:Legend2Шаблон:·Шаблон:Legend2

Geographos orbits the Sun at a distance of 0.8–1.7 AU once every 1 years and 5 months (508 days). Its orbit has an eccentricity of 0.34 and an inclination of 13° with respect to the ecliptic.[3] Its orbit is well-determined for the next several hundred years. Due to its high eccentricity, Geographos is also a Mars-crosser asteroid. The body's observation arc begins at Palomar, two weeks prior to its official discovery observation.[1]

Close approaches

As a potentially hazardous asteroid, Geographos has a minimum orbital intersection distance (MOID) with Earth of less than 0.05 AU and a diameter of greater than 150 meters. The Earth-MOID is currently Шаблон:Convert, which translates into 11.7 lunar distances.[3] In 1994, Geographos made its closest approach to Earth in two centuries at 5.0 Gm – which will not be bettered until 2586.[4]

Failed Clementine mission

Geographos was to be explored by the U.S.'s Clementine mission which was launched in January 1994. However, a malfunction in the spacecraft ended the mission before it could approach the asteroid.[5]

Physical characteristics

Spectral type

In the Tholen and SMASS classification, Geographos is an S-type asteroid.[3] This means that it is highly reflective and composed of nickel-iron mixed with iron- and magnesium-silicates.

Rotation period

Since the 1970s, several rotational lightcurve of Geographos have been obtained from photometric observations. Lightcurve analysis gave a rotation period (retrograde sense of rotation) between 5.222 and 5.224 hours with a very high brightness variation between 1.02 and 2.03 magnitude (Шаблон:Small).[6][7][8][9][10][11]Шаблон:Efn

The Yarkovsky effect is causing a decrease in the orbital semimajor axis of Шаблон:Val,[12] while the YORP effect is increasing the asteroid's rotation at the rate of Шаблон:Val.[13]

Spin axis

Several lightcurve were also modeled from the abundant photometric observations. In 1994 and 1995, Polish astronomers obtained a concurring period 5.223328 hours and found a spin axis of (54.0°, −52.0°) in ecliptic coordinates (λ, β) (Шаблон:Small).[14][15] Radiometric observations gave a period of 5.223327 hours and a pole of (55.0°, −46.0°).[16] Two other international studies obtained a period of 5.223326 hours and a pole at (56.0°, −47.0°) and (55.0°, −45.0°), respectively (Шаблон:Small).[17][18]

Shape and structure

The light curve shows a high amplitude, indicative of its elongated shape, measuring 5.0×2.0×2.1 kilometers, which corresponds to a mean-diameter of 2.5 km.[16]

The interior of the asteroid probably has a rubble-pile structure. The asteroid's high thermal inertia indicates the surface is most likely a mix of fine grains and large rocks and boulders.[12] During the asteroid's close approach to Earth in 1994, a radar study of it was conducted by the Deep Space Network at the Goldstone Observatory, California. The resultant images show Geographos to be the most elongated object in the Solar System.[4]

Diameter and albedo

According to the observations with the Goldstone Observatory and the space-based surveys carried out by the Infrared Astronomical Satellite IRAS and the NEOWISE mission of the Wide-field Infrared Survey Explorer, Geographos measures between 1.77 and 2.56 kilometers in diameter and its surface has an albedo between 0.26 and 0.3258.[19][20][21][22][16] The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.26 and a diameter of 2.5 kilometers based on an absolute magnitude of 15.09.[23]

Naming

This minor planet was named after the National Geographic Society, in recognition of its contribution to astronomy by supporting the National Geographic Society – Palomar Observatory Sky Survey (NGS-POSS), which produced a photographic atlas of the entire northern sky in the 1950s. NGS-POSS was headed by the second discoverer, Rudolph Minkowski. The Greek word Шаблон:Lang means geographer (from geo– 'Earth' + Шаблон:Lang 'drawer/writer').[2] The official Шаблон:MoMP was published by the Minor Planet Center in August 1956 (Шаблон:Small).[24]

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator

Шаблон:Authority control

  1. 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  2. 2,0 2,1 Ошибка цитирования Неверный тег <ref>; для сносок springer не указан текст
  3. 3,0 3,1 3,2 Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  4. 4,0 4,1 Ошибка цитирования Неверный тег <ref>; для сносок Ostro-1996 не указан текст
  5. NASA - Clementine
  6. Ошибка цитирования Неверный тег <ref>; для сносок Higgins-2008b не указан текст
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  12. 12,0 12,1 Ошибка цитирования Неверный тег <ref>; для сносок Rozitis-2014 не указан текст
  13. Шаблон:Cite journal
  14. Ошибка цитирования Неверный тег <ref>; для сносок Michalowski-1994 не указан текст
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  24. Ошибка цитирования Неверный тег <ref>; для сносок DoMP-Circular-dates не указан текст