File:How Sunlight Pushes Asteroids
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[edit]| DescriptionEzh3 metro train in a tunnel.webm | English: Near-Earth asteroids like Bennu pose a potential danger to our planet, so it's important to predict their orbits with great accuracy. Unfortunately, a phenomenon called the Yarkovsky effect can make these predictions difficult over long time periods. How does this effect work? When sunlight strikes a rotating asteroid, the dayside heats up; as the asteroid turns, the night side cools and releases the heat, exerting a small thrust that can change the asteroid's direction over time. In order to learn more about this process on asteroid Bennu, NASA is sending a spacecraft called OSIRIS-REx to make detailed observations of Bennu's shape, brightness, and surface features. These factors are thought to influence the Yarkovsky effect, and understanding how will enable scientists to better predict the orbit of Bennu and other near-Earth asteroids. |
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| Date | ||||
| Source | NASA | |||
| Author | NASA | |||
| Permission (Reusing this file) |
This file is licensed under Public Domain (US Government Work). You are free to share and adapt this work as long as attribution is provided and changes are indicated. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:39, 1 February 2026 | 1 min 37 s, 1,920 Ã 1,080 (23.36 MB) | Xenotron (talk | contribs) | Imported media from uploads:5fafaed2-ff50-11f0-afed-560e478790eb |
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File:Ezh3 metro train in a tunnel.webm