Archivo de imágenes de Hubble
Sistema binario de asteroides 2006 VW139/288P
This set of Hubble Space Telescope photos reveals two asteroids orbiting each other that have comet-like features. These include a bright halo of material, called a coma, and a long tail of dust. The asteroid pair, called 2006 VW139/288P, was observed in September 2016 just befor...
- Fecha
- Jan 1, 2017
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2017-32-4067-image
This set of Hubble Space Telescope photos reveals two asteroids orbiting each other that have comet-like features. These include a bright halo of material, called a coma, and a long tail of dust. The asteroid pair, called 2006 VW139/288P, was observed in September 2016 just before the asteroid made its closest approach to the Sun. The photos revealed ongoing activity in the binary system. The apparent movement of the tail is a projection effect due to the relative alignment between the Sun, Earth, and 2006 VW139/288P changing between observations. The tail orientation is also affected by a change in the particle size. Initially, the tail was pointing towards the direction where comparatively large (about 1 millimeter in size) dust particles were emitted in late July. However, from Sept. 20 on, the tail began to point in the opposite direction from the Sun, where small (about 10 microns in size) particles are blown away from the nucleus by radiation pressure.
Credits
NASA, ESA, and J. Agarwal (Max Planck Institute for Solar System Research)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | 288P |
| Object Description | A binary asteroid system |
| About The Data | |
| Data Description | Data were provided by the HST proposals , , , . |
| Instrument | WFC3/UVIS |
| Exposure Dates | August 22 - September 29, 2016 |
| Filters | F606W |
| About The Image | |
| Color Info | These images represent several exposures acquired by the WFC3/UVIS instrument on the Hubble Space Telescope. Color has been applied to the grayscale (black&white) images; the brightness maps to different color values. |
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Fuente
La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov