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Observatories and Instruments

Very Long Baseline Array

Ground-Based Radio and Millimeter Observatories

A US National Radio Astronomy Observatory network of ten identical 25-meter radio dishes spread from Hawaii to the US Virgin Islands, their signals combined after the fact to synthesize a telescope effectively as large as the whole continent. Completed in 1993, it delivers among the sharpest angular resolution of any astronomical instrument ever built.

Facts
Classification
Observing Band
Radio 1
Operational
from 1993 2
Connections

Operated By

Source Very Long Baseline Array (Wikipedia)
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Located In

Also in Geography Atlas: where this subject is located.

Sources
1. Wikipedia (space and spaceflight articles)
Wikimedia Foundation
2. Very Long Baseline Array (Wikipedia)
  • Very Long Baseline Array, Wikipedia - lead section, observing band (radio)
    The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO).
  • Article text, operational-start-year
    it was completed in May 1993
  • In Group: Radio and Millimetre Interferometer Arrays, Lead sentence
    The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO).
  • Operated By: National Radio Astronomy Observatory, Article text: operator
    The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro, New Mexico, as a part of the National Radio Astronomy Observatory (NRAO).
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