Answer
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Hint: To measure distances in the universe, Arcseconds and Parsecs are both used. An arcsecond is a way of measuring the distances in space between objects based on Earth observations, while a parsec tells you how far away from Earth the object is.
Complete answer:
1.Divide 1 by the parallax arc-seconds to calculate the distance to a star in parsecs. Divide the number by 1,000, first to calculate with milliarcseconds, then divide 1 by the result.
2.The units of length are parseconds and light years. In these units, the distances between planets and stars in outer space are measured.
3.Between these two measurements you can convert because one parsec is equal to the one-arcsecond parallax.
4.Your position when you observe a star and the position of the Earth in its orbit affects your view of the surroundings of the star and its location in the sky.
5.The change of perspective is known as the parallax that you measure, three months earlier or later, as the angle between the position of the Earth now the star, and the position of the Earth. Being an angle, in degrees of arc, it has units.
Note:
Since parallax measurements can end up being a small fraction of a degree, you usually use arc seconds, also known as arcseconds (one 3,600th of a degree). In order to figure out the distance to the star, expressed in parsecs, derived from one-arcsecond parallax," you need this value. The distance that subtends a parallax angle of one arc-second is one parsec.
Complete answer:
1.Divide 1 by the parallax arc-seconds to calculate the distance to a star in parsecs. Divide the number by 1,000, first to calculate with milliarcseconds, then divide 1 by the result.
2.The units of length are parseconds and light years. In these units, the distances between planets and stars in outer space are measured.
3.Between these two measurements you can convert because one parsec is equal to the one-arcsecond parallax.
4.Your position when you observe a star and the position of the Earth in its orbit affects your view of the surroundings of the star and its location in the sky.
5.The change of perspective is known as the parallax that you measure, three months earlier or later, as the angle between the position of the Earth now the star, and the position of the Earth. Being an angle, in degrees of arc, it has units.
Note:
Since parallax measurements can end up being a small fraction of a degree, you usually use arc seconds, also known as arcseconds (one 3,600th of a degree). In order to figure out the distance to the star, expressed in parsecs, derived from one-arcsecond parallax," you need this value. The distance that subtends a parallax angle of one arc-second is one parsec.
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