Английская Википедия:469219 Kamoʻoalewa

Содержание

Текст

Текст

Текст

Текст

Текст

Текст

Текст

Текст

Текст

469219 Kamoʻoalewa (Шаблон:IPAc-en), provisionally designated Шаблон:Mp, is a very small asteroid, fast rotator and near-Earth object of the Apollo group, approximately Шаблон:Convert in diameter. At present it is a quasi-satellite of Earth, and currently the second-smallest, closest, and most stable known such quasi-satellite (after 2023 FW13). The asteroid was discovered by Pan-STARRS at Haleakala Observatory on 27 April 2016. It was named Шаблон:MoMP, a Hawaiian word that refers to an oscillating celestial object. The Earth-like orbit and lunar-like silicates may be a result of it being lunar ejecta.

Discovery and naming

Kamoʻoalewa was first spotted on 27 April 2016, by the Pan-STARRS 1 asteroid survey telescope on Haleakalā, Hawaii, that is operated by the University of Hawaii's Institute for Astronomy and funded by NASA's Planetary Defense Coordination Office. The name Kamoʻoalewa is derived from the Hawaiian words ka 'the', moʻo 'fragment', referring to it being a piece broken off a larger object, a 'of', and lewa 'to oscillate', referring to its motion in the sky as viewed from Earth. The official Шаблон:MoMP was published by the Minor Planet Center on 6 April 2019 (Шаблон:Small).

Orbit and classification

Kamoʻoalewa orbits the Sun at a distance of 0.90–1.10 AU. Although the period as of 2022 is about 366 days, its longer-term average period is closer to 365 days since it is a quasi-satellite of Earth and will continue to be so for hundreds of years. Its orbit has an eccentricity of 0.10 and an inclination of 8° with respect to the ecliptic. It has an Earth minimum orbital intersection distance of Шаблон:Convert that translates into 13 lunar distances. This distance is well outside of Earth's Hill sphere of Шаблон:Convert.

Quasi-satellite of Earth

Файл:Asteroid2016HO3-SunEarthOrbit.webm

The oscillating path of asteroid Kamoʻoalewa as it orbits around the Sun. The traced path of Kamoʻoalewa makes it appear as a constant companion of the Earth.

As it orbits the Sun, Kamoʻoalewa appears to circle (highly elliptically) around Earth as well. The object is beyond the Hill sphere of Earth and the Sun exerts a much stronger pull on it than Earth does. Although it is too distant to be considered a true natural satellite of Earth, it is the best and most stable example to date of a near-Earth companion, or quasi-satellite.

Paul Chodas, manager of NASA's Center for Near-Earth Object (NEO) Studies at the Jet Propulsion Laboratory in Pasadena, California, commented on the orbit:

In its yearly trek around the Sun, Kamoʻoalewa spends approximately half of the time closer to the Sun than Earth is (that is, the asteroid is inside the Earth's orbit) and passes ahead of our planet, and approximately half of the time farther away (crosses outside Earth's orbit), causing it to fall behind. Also, its orbit is tilted a little, causing it to bob up and then down once each year through Earth's orbital plane. In effect, this small asteroid is caught in a game of leap frog with Earth that will last for hundreds of years.

Chodas explained how the asteroid's orbit also undergoes a slow, back-and-forth twist over multiple decades: Шаблон:Blockquote

In terms of orbit, it currently is the most stable among the quasi-satellites of Earth that have been discovered and will remain in that orbit for about the next 300 years. The closest Earth approach was on 27 December 1923 at Шаблон:Convert. By late May 2369 the asteroid will be Шаблон:Convert from Earth. The Earth-like orbit may be a result of it being lunar ejecta.

Physical characteristics

The size of Kamoʻoalewa has not yet been firmly established, but it is approximately Шаблон:Convert. Based on an assumed standard albedo for stony S-type asteroids of 0.20, its absolute magnitude of 24.3 corresponds to a Шаблон:Convert diameter.

Photometric observations in April 2017 revealed that Kamoʻoalewa is a fast rotator. Lightcurve analysis gave a rotation period of Шаблон:Convert and a brightness variation of Шаблон:Val magnitude (Шаблон:Small).Шаблон:Refn

In 2021, a comprehensive physical characterization of Kamoʻoalewa was conducted using the Large Binocular Telescope and the Lowell Discovery Telescope, which found that the asteroid is composed of lunar-like silicates and may be an impact fragment from the Moon.

Exploration

Proposed missions

During the 2017 Astrodynamics Specialist Conference held in Stevenson in the U.S. state of Washington, a team composed of graduate research assistants from the University of Colorado Boulder and the São Paulo State University (UNESP) was awarded for presenting a project denominated "Near-Earth Asteroid Characterization and Observation (NEACO) Mission to Asteroid (469219) Шаблон:Mp", providing the first baselines for the investigation of this celestial object using a spacecraft. Recently, another version of this work was presented adopting different constraints in the dynamics.

The China National Space Administration (CNSA) is planning a robotic mission that would return samples from Kamoʻoalewa. This mission, Tianwen-2, is planned to launch in 2025.

See also

• Arjuna asteroid
• Natural satellite
• Quasi-satellite
• 3753 Cruithne
• 6Q0B44E
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl
• Шаблон:Mpl, a quasi-satellite of Venus, and the first quasi-satellite discovered around any major planet

External links

• Asteroid 2016 HO3 - Earth's Constant Companion NASA Jet Propulsion Laboratory, 23 June 2016
• Asteroid Lightcurve Database (LCDB), query form (info Шаблон:Webarchive)
• Шаблон:NeoDys
• Шаблон:ESA-SSA
• Шаблон:JPL small body