File:AreciboOrbitalFitGaiaDR3.jpg
Size of this preview: 800 × 442 pixels. Other resolutions: 320 × 177 pixels | 640 × 354 pixels | 1,024 × 566 pixels | 1,280 × 707 pixels | 2,342 × 1,294 pixels.
Original file (2,342 × 1,294 pixels, file size: 192 KB, MIME type: image/jpeg)
 | This is a file from the Wikimedia Commons. Information from its description page there is shown below. Commons is a freely licensed media file repository. You can help. |
Summary
| Description |
English: The case of the asteroid 4337 Arecibo is emblematic. The presence of a companion has not been discovered by Gaia, but from the ground by two stellar occultations. A first look in Gaia data revealed the periodic oscillation of the asteroid trajectory, thus resulting in the first astrometric signature detected for an asteroid satellite. |
| Date | |
| Source | https://www.cosmos.esa.int/web/gaia/dr3-solar-system-objects |
| Author | Paolo Tanga, et al. 2022, ESA/Gaia/DPAC |
Licensing
This file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
- share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 03:35, 17 June 2022 | | 2,342 × 1,294 (192 KB) | Nrco0e | Uploaded a work by Paolo Tanga, et al. 2022, ESA/Gaia/DPAC from https://www.cosmos.esa.int/web/gaia/dr3-solar-system-objects with UploadWizard |
File usage
The following page uses this file:
