A distance of one million parsecs (approximately 3,262,000 light-years) is commonly denoted by the megaparsec(Mpc).
Sirius is approximately 2.6 parsecs or 8.6 light years away from Earth.
The distance to the star can be calculated using the parallax angle (in arcseconds) and the formula: distance (in parsecs) = 1 / parallax angle (in arcseconds). Given a parallax of 0.75 arcseconds, the star is approximately 1.33 parsecs away. Converting parsecs to light years (1 parsec ≈ 3.26 light years), the star is about 4.34 light years away.
Jupiter is 483.6 million miles (778.3 million km) away from the Sun. (The given figure is the average distance)
No Regulus or Alpha Leonis is 23.8 parsecs from the Earth.
Alpha Centauri is approximately 1.34 parsecs away from Earth. This distance makes it the closest star system to our Solar System. In light-years, this translates to about 4.37 light-years.
30.659 parsecs
Rigel is 260 +/-20 parsecs away.
Sirius is approximately 2.6 parsecs or 8.6 light years away from Earth.
The distance to the star can be calculated using the parallax angle (in arcseconds) and the formula: distance (in parsecs) = 1 / parallax angle (in arcseconds). Given a parallax of 0.75 arcseconds, the star is approximately 1.33 parsecs away. Converting parsecs to light years (1 parsec ≈ 3.26 light years), the star is about 4.34 light years away.
Denebola is located approximately 36.9 light-years away from Earth.
Light years, parsecs, and kiloparsecs. Light years and parsecs are used to measure distances between neighbouring star system's, kiloparsecs are used to measure distances within a galaxy.
The standard distance is 10 parsecs. At this distance the star's apparent magnitude equals its absolute magnitude. A star 100 parsecs away has an absolute magnitude 5 magnitudes brighter than its apparent magnitude. 1 parsec is 3.26 light-years.
It is 260 +/- 20 parsecs away.
I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.I assume you mean the parallax. If the parallax is 0.1 arc-seconds, then the distance is 1 / 0.1 = 10 parsecs.
1 megaparsec is a distance, equal to 1 million parsecs. 1 parsec is the distance of about 3.26 light years. It's the distance from us that an object is if ... in six months, when the Earth moves from one side of its orbit to the other side ... the object 1 parsec away appears to shift its position against the 'distant background' objects by 1 second = 1/3,600 of a degree.
Jupiter is 483.6 million miles (778.3 million km) away from the Sun. (The given figure is the average distance)
If a star has a parallax of 0.05 (seconds of arc) then its distance in light years is about 65.2 light years. A little more detail, if required: Distance to a star (in parsecs) = 1/parallax (in seconds of arc). So, in this case: Distance = 1/0.05 = 20 parsecs. A parsec is a distance of about 3.26 light years. So, that means the answer is about 20 x 3.26 light years. That's about 65.2 light years.