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Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect
by
Benner, Lance A.M
, Ostro, Steven J
, Magri, Christopher
, Lowry, Stephen C
, Fitzsimmons, Alan
, Scheeres, Daniel J
, Taylor, Patrick A
, Vokrouhlický, David
, Pravec, Petr
, Nolan, Michael C
, Margot, Jean-Luc
, Giorgini, Jon D
in
Acceleration
/ Asteroids
/ Asteroids (minor planets)
/ Astronomy
/ Cosmology
/ Double stars
/ Earth, ocean, space
/ Exact sciences and technology
/ Light curves
/ Mass, size; gravitational fields; rotation; orbits
/ Modeling
/ Near Earth objects
/ Observational astronomy
/ Planetary, asteroid, and satellite characteristics and properties
/ Planets, their satellites and rings. Asteroids
/ prediction
/ Radar
/ Radar echoes
/ Radar tracking
/ Rotation
/ Signal bandwidth
/ solar radiation
/ Solar system
/ Theory
/ torque
2007
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Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect
by
Benner, Lance A.M
, Ostro, Steven J
, Magri, Christopher
, Lowry, Stephen C
, Fitzsimmons, Alan
, Scheeres, Daniel J
, Taylor, Patrick A
, Vokrouhlický, David
, Pravec, Petr
, Nolan, Michael C
, Margot, Jean-Luc
, Giorgini, Jon D
in
Acceleration
/ Asteroids
/ Asteroids (minor planets)
/ Astronomy
/ Cosmology
/ Double stars
/ Earth, ocean, space
/ Exact sciences and technology
/ Light curves
/ Mass, size; gravitational fields; rotation; orbits
/ Modeling
/ Near Earth objects
/ Observational astronomy
/ Planetary, asteroid, and satellite characteristics and properties
/ Planets, their satellites and rings. Asteroids
/ prediction
/ Radar
/ Radar echoes
/ Radar tracking
/ Rotation
/ Signal bandwidth
/ solar radiation
/ Solar system
/ Theory
/ torque
2007
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Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect
by
Benner, Lance A.M
, Ostro, Steven J
, Magri, Christopher
, Lowry, Stephen C
, Fitzsimmons, Alan
, Scheeres, Daniel J
, Taylor, Patrick A
, Vokrouhlický, David
, Pravec, Petr
, Nolan, Michael C
, Margot, Jean-Luc
, Giorgini, Jon D
in
Acceleration
/ Asteroids
/ Asteroids (minor planets)
/ Astronomy
/ Cosmology
/ Double stars
/ Earth, ocean, space
/ Exact sciences and technology
/ Light curves
/ Mass, size; gravitational fields; rotation; orbits
/ Modeling
/ Near Earth objects
/ Observational astronomy
/ Planetary, asteroid, and satellite characteristics and properties
/ Planets, their satellites and rings. Asteroids
/ prediction
/ Radar
/ Radar echoes
/ Radar tracking
/ Rotation
/ Signal bandwidth
/ solar radiation
/ Solar system
/ Theory
/ torque
2007
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Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect
Journal Article
Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect
2007
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Overview
Radar and optical observations reveal that the continuous increase in the spin rate of near-Earth asteroid (54509) 2000 PH5 can be attributed to the Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect, a torque due to sunlight. The change in spin rate is in reasonable agreement with theoretical predictions for the YORP acceleration of a body with the radar-determined size, shape, and spin state of 2000 PH5. The detection of asteroid spin-up supports the YORP effect as an explanation for the anomalous distribution of spin rates for asteroids under 10 kilometers in diameter and as a binary formation mechanism.
Publisher
American Association for the Advancement of Science,The American Association for the Advancement of Science
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