Archivo de imágenes de Hubble
Galaxia espiral barrada NGC 1512 en luz infrarroja
The deeper orange (1.6 microns) moves farther into the infrared region of the spectrum. Image taken with HST's Near Infrared Camera and Multi-Object Spectrometer (NICMOS). CreditsNASA, ESA, and D. Maoz (Tel-Aviv University and Columbia University)
- Fecha
- Jan 1, 2001
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2001-16-1065-image
The deeper orange (1.6 microns) moves farther into the infrared region of the spectrum. Image taken with HST's Near Infrared Camera and Multi-Object Spectrometer (NICMOS).
Credits
NASA, ESA, and D. Maoz (Tel-Aviv University and Columbia University)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | NGC 1512 |
| Object Description | Barred spiral galaxy |
| R.A. Position | 04h 3m 54.29s |
| Dec. Position | -43° 20' 56.0" |
| Constellation | Horologium |
| Distance | 9.2 million pc (30 million light-years) |
| Dimensions | The galaxy is 70,000 light-years across. The circumnuclear starburst ring is 2,400 light-years wide. |
| About The Data | |
| Data Description | Principal Astronomers: D. Maoz (Tel-Aviv University/Columbia University), A. J. Barth (Harvard CfA), L. C. Ho (Carnegie Obs.), A. Sternberg (Tel-Aviv University and A. V. Filippenko (UC Berkeley). Members of the group of scientists involved in these observations are: Dan Maoz (Tel-Aviv University, Israel and Columbia University, USA), Aaron J. Barth (Harvard-Smithsonian Center for Astrophysics, USA), Luis C. Ho (The Observatories of the Carnegie Institution of Washington, USA), Amiel Sternberg (Tel-Aviv University, Israel) and Alexei V. Filippenko (University of California, Berkeley, USA). |
| Instrument | HST>NICMOS |
| Exposure Dates | July 29, 1998 |
| Filters | F160W (1.6mm), and F187W (1.8mm) |
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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