| Revision as of 09:22, 30 October 2003 editAlex.tan (talk | contribs)Extended confirmed users5,403 edits same light gathering as 16m telescope← Previous edit | Revision as of 18:15, 8 November 2003 edit undoMav (talk | contribs)Extended confirmed users77,874 editsmNo edit summaryNext edit → | ||
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| In its full interferometric operating mode, the four telescopes provide the same light gathering ability as a single 16m telescope, making it the largest optical telescope in the world. The VLT is intended to achieve an effective ] of 0.001 ] at a ] of 1 µm. This is an angle of 0.000000005 ]s, equivalent to resolving a target 2 meters across at the distance between the ] and ]. | In its full interferometric operating mode, the four telescopes provide the same light gathering ability as a single 16m telescope, making it the largest optical telescope in the world. The VLT is intended to achieve an effective ] of 0.001 ] at a ] of 1 µm. This is an angle of 0.000000005 ]s, equivalent to resolving a target 2 meters across at the distance between the ] and ]. | ||
| This should easily resolve the 5-metre wide Lunar Module bases left on the Moon by the ] moon missions, and a group of European scientists intends to do just that to challenge |
This should easily resolve the 5-metre wide Lunar Module bases left on the Moon by the ] moon missions, and a group of European scientists intends to do just that to challenge ]. | ||
| See also: | See also: | ||
Revision as of 18:15, 8 November 2003
The Very Large Telescope (VLT) consist of four separate optical telescopes that each have 8.4 meter aperture. The VLT is a project of the European Southern Observatory organization.
It is located at the Paranal Observatory on Cerro Paranal, a 2,635-m high mountain in the Atacama desert in northern Chile.
The VLT consists of a cluster four of large telescopes, and an interferometer (VLTI) which will be used to resolve fine features. The telescopes have been named after the names of some astronomical objects in the local Mapuche language: Antu (The Sun), Kueyen (The Moon), Melipal (The Southern Cross), and Yepun (Venus)
The VLT can be operated in three modes:
- as a set of independent telescopes
- as a single large incoherent instrument, for extra light-gathering capacity
- as a single large coherent interferometric instrument, for extra resolution
In its full interferometric operating mode, the four telescopes provide the same light gathering ability as a single 16m telescope, making it the largest optical telescope in the world. The VLT is intended to achieve an effective angular resolution of 0.001 arcsecond at a wavelength of 1 µm. This is an angle of 0.000000005 radians, equivalent to resolving a target 2 meters across at the distance between the Earth and Moon.
This should easily resolve the 5-metre wide Lunar Module bases left on the Moon by the Apollo moon missions, and a group of European scientists intends to do just that to challenge Apollo moon landing hoax accusations.
See also: