File:Solar Nebular Theory and the Formation of the Solar System.jpg
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Summary
| Description | English: Following a supernova, dispersed clouds of gas and dust begin to condense. Eventually rotation and gravity form a flat disk-like solar system with accreting protoplanets. |
| Date | 20 June 2022 |
| File source | https://www.phy.olemiss.edu/~luca/astr/Topics-Solar/Formation-N.html |
| Author | Luca Bombelli |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 03:10, 25 June 2022 | | 354 × 394 (22 KB) | AllyPatinios (talk | contribs) | Uploaded a work by Luca Bombelli from https://www.phy.olemiss.edu/~luca/astr/Topics-Solar/Formation-N.html with UploadWizard |
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