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- Planetesimal - Wikipedia
A planetesimal is a solid object arising during the accumulation of orbiting bodies whose internal strength is dominated by self-gravity and whose orbital dynamics is not significantly affected by gas drag
- Planetesimal | Astronomy, Solar System Planet Formation | Britannica
Planetesimal, one of a class of bodies that are theorized to have coalesced to form Earth and the other planets after condensing from concentrations of diffuse matter early in the history of the solar system
- Astronomer Explains What is a Planetesimal - Little Astronomy
An object is considered a planetesimal when it is larger than 1 kilometer long (0 6 miles) and can be found orbiting a star This is where the confusion begins as that is also the same definition of an asteroid
- Planetesimal Formation - The Stephen W. Hawking Center for Microgravity . . .
Planetesimal Formation Planetesimals are the building blocks of planets Asteroids and comets are leftover planetesimals from the time of formation of our own solar system The formation of km-sized or larger planetesimals remains an open problem in planet formation theories
- What Is a Planetesimal? Space Rocks that Assemble Planets
What Is a Planetesimal? A planetesimal is a small celestial body that forms during the early stages of planetary formation in a protoplanetary disk These objects are typically composed of dust, ice, and other materials, ranging in size from several miles to hundreds of miles in diameter
- Planetesimals - Universe Today
According to the planetesimal hypothesis, when a planetary system is forming, there is a protoplanetary disk with materials from the nebulae from which the system came
- 36 Facts About Planetesimals
The Rosetta mission studied a planetesimal The European Space Agency's Rosetta spacecraft studied comet 67P Churyumov-Gerasimenko, providing valuable data on planetesimals
- Planetesimal Theory of Planet Formation - BrightHub
Planetesimal theory describes how the terrestrial planets and the Jovian planets formed From the collision and accumulation of planetesimals in the solar nebula larger bodies formed and eventually clumped together to form planets This theory was first proposed by Viktor Safronov
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