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Apr 16, 2024 · PDF | Thermally induced torque, the so-called YORP effect has decelerated the rotation of asteroid Ryugu since the rapid rotation era in ...
Jan 17, 2024 · We simulated the asteroid's close Earth approaches from 2001 to 2005, showing that gravitational torques cannot explain the observed spin rate ...
Missing: 350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History | Show results with:350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History
Jan 10, 2024 · The net effect of many small interactions, taken in isolation, is to cause the asteroid to spin at a faster rate—although this must be balanced ...
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Sep 26, 2019 · The distribution of rotation rates of small (D = 3–15 km) main-belt asteroids is analyzed in the context of the probable influence of solar ...
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(1) Trauma to the Earth, such as a large meteorite collision [124, 125], could in principle disrupt convection in the sub-shell of the georeactor, ...
Missing: 350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History | Show results with:350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History
The rotation rate distribution of small Main Belt asteroids is dominated by YORP and collisions. These mechanism act differently depending on the size of ...
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The impact of a meteoroid onto an asteroid transfers linear and angular momentum to the larger body, which may affect its orbit and its rotational state.
Missing: 350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History | Show results with:350987795_YORP_Effect_on_Asteroid_162173_Ryugu_Implications_for_the_Dynamical_History
The asteroid belt size distribution was shaped by collisions grinding the population into smaller bodies via cratering or fragmentation. At the small size ...
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We report on the formation of graphitized carbon on GaAs(100) surfaces by molecular beam epitaxy. We grew highly carbon-doped GaAs on AlAs, which was then ...
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