Angular resolution: Difference between revisions

Revision as of 01:24, 27 September 2022

Revision as of 01:27, 27 September 2022

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! Name || class="unsortable"| Image ||data-sort-type="number"| Angular resolution ([[arc seconds]])|| Wavelength || Type || Site || Year

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| [[Global mm-VLBI Array]] (successor to the ''Coordinated Millimeter VLBI Array'')|| || 0.000012 || radio || [[very long baseline interferometry]] array of different [[radio telescope]]s || a range of locations on Earth and in space<ref name="Max Planck Institute for Radio Astronomy 2022">{{cite web | title=Images at the Highest Angular Resolution in Astronomy | website=Max Planck Institute for Radio Astronomy | date=2022-05-13 | url=https://www.mpifr-bonn.mpg.de/pressreleases/2022/2 | access-date=2022-09-26}}</ref> || 2002 - 

|-

| [[Very Large Telescope]]/[[PIONIER (VLTI)|PIONIER]]|| [[File:Paranal and the Pacific at sunset (dsc4088, retouched, cropped).jpg|50px]] || 0.001 || light || largest [[optical astronomy|optical]] array of 4 [[reflecting telescope]]s || [[Paranal Observatory]], [[Antofagasta Region]], Chile || 2002/2010 -

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| [[Hubble Space Telescope]]|| [[File:HST.jpg|50px]] || 0.03 || light || [[space telescope]] || [[Earth orbit]] || 1990 -

|}