Sentence examples similar to parallax second from inspiring English sources

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parallax second

noun

A unit of length, used in astronomy, defined as the distance from the Earth of an object that exhibits a parallax of 1 arcsecond. It is approximately equal to 3.08568025 × 1013 kilometers, or 3.2616 light-years.

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These real motions as well as the apparent ones due to parallax, first measured by the German astronomer Friedrich Bessel in 1838 were not detected by the ancients because of the enormous distance scale of the stellar universe.

Its parallax, first taken at the Cape of Good Hope by Henderson in 1839, and later by Gill and Elkin, and now fixed at 0ʺ.75, shows a distance equal to that traveled by light in 4⅓ years.

Currently showing at The Tufts University Art Gallery in Medford, Massachusetts until the beginning of December, this is Parallax's first museum debut in the U.S., having been previously shown at influential art institutions including the Guggenheim Museum in Bilbao and as a part of the Sharjah Biennial.

For 118,000 selected stars, Hipparcos measured their parallax accurate to.001 second of arc.

For example, the nearest star, Proxima Centauri, which is part of the Alpha Centauri triple-star system, has a parallax of 0.769 second of arc; hence, its distance from the Sun and Earth is 1.30 parsec.

The transverse (or tangential) velocity, T, is given by T = V sin λ = 4.74 μ/p where p is the star's parallax in arc seconds.

The transverse (or tangential) velocity, T, is given byT = V sin λ = 4.74 μ/p where p is the star's parallax in arc seconds.

The first parallax measurement of Wolf 359 was reported in 1928 from the Mount Wilson Observatory, yielding an annual shift in the star's position of 0.407 ± 0.009 arcseconds.

Fellows previously brought us through key tactics he uses to achieve a 2.5D animation (also called parallax) in our first video profile of the artist.

This unit of distance is termed the parsec, defined as the distance of an object whose parallax equals one arc second.

Also, were earlier attempts to measure parallax of Sirius: by the second Cassini (6 seconds); by some astronomers (including Nevil Maskelyne) using Lacaille's observations made at the Cape of Good Hope (4 seconds); by Piazzi (the same amount); using Lacaille's observations made at Paris, more numerous and certain than those made at the Cape (no sensible parallax); by Bessel (no sensible parallax).

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