Angular diameter
The angular diameter of an object as seen from a given position is the diameter measured as an angle. It satisfies the formula delta = rctan (diameter/ distance).
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In astronomy the size of objects in the sky are often measured in terms of their angular diameter as seen from Earth, rather than their actual size.
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The angular diameter of Earth's orbit around the Sun, from a distance of one parsec, is 2" (two arcseconds).
Related Topics:
Parsec - Arcsecond
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The angular diameter of the Sun, from a distance of one lightyear, is 0.03", of the Earth 0.0003".
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This table shows the angular sizes of the most important Solar System bodies.
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Sun30'
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Moon29' - 33'
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Venus10" - 58"
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Jupiter 32" - 49"
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Saturn 16" - 20"
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Mars 4" - 16"
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Uranus 3" - 4"
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Neptune 2"
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- Alpha Centauri A: ca. 0.007"
- Sirius: ca. 0.007"
Thus the angular diameter of the Sun is ca. 250,000 that of Sirius (it has twice the diameter and the distance is 500,000 times as much; the Sun is 10,000,000,000 times as bright, corresponding to an angular diameter ratio of 100,000, so Sirius is roughly 6 times as bright per unit solid angle).
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The angular diameter of the Sun is also ca. 250,000 that of Alpha Centauri A (it has the same diameter and the distance is 250,000 times as much; the Sun is 40,000,000,000 times as bright, corresponding to an angular diameter ratio of 200,000, so Alpha Centauri A is a little brighter per unit solid angle).
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The angular diameter of the Sun is about the same as that of the Moon (the diameter is 400 times as large and the distance also; the Sun is 200,000-500,000 times as bright as the full Moon (figures vary), corresponding to an angular diameter ratio of 450-700, so a celestial body with a diameter of 2.5-4" and the same brightness per unit solid angle would have the same brightness as the full Moon).
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