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Summary
| Description |
English: Dusty proplyd in the star cluster NGC 1977, which appears as a star leaving a red tail behind. The external evaporation of dust from the disk of this object is caused by nearby OB-stars. The dust is then swept away by the nearby OB-star 42 Orionis, forming a tail in the wake of the young star.
Image Credit: NASA Spitzer Space Telescope Filters: 4.5, 8.0 and 24 Micron |
| Date | |
| Source | Own work |
| Author | Meli thev |
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| Annotations | This image is annotated: View the annotations at Commons |
File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 18:32, 15 May 2023 | | 418 × 438 (47 KB) | Meli thev | Uploaded own work with UploadWizard |
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