Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). Based on parallax measurements, it is approximately 470 light-years from the Sun..
All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 4,774,004.69.km. An Astronomical Unit is the distance between Earth and the Sun. Theta Scorpii is an evolved bright yellow giant star of spectral type F0 II.
The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -7.60000 km/s with an error of about 3.90 km/s . By using our services, you agree to our use of cookies. Based on the spectral type, we can deduce that the surface temperature of the star is in the order of between between 10,000 and 25,000K based on the notes from Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out.
Its distance from the Sun is about 474 light-years, as determined by parallax measurements. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. In the case of a star, its the galactic centre. Apparent Magnitude is also known as Visual Magnitude. A faint star will have a high number. MU-1 SCO (Mu-1 Scorpii). A faint star will have a high number. RoCookies help us deliver our services.
Using the 2007 distance, the star is roughly 31,684,116.11 Astronomical Units from the Earth/Sun give or take a few. Mu Scorpii: | The |Bayer designation| |Mu Scorpii| (μ Sco, μ Scorpii) is shared by two |star systems|, ... World Heritage Encyclopedia, the aggregation of the largest online encyclopedias available, and the most definitive collection ever assembled. For Xamidimura, the location is 16h 51m 52.24 and -38° 02` 50.4 . Its variable/pulsating period lasts for 1.4 days (variability). It has an apparent visual magnitude of +3.56, which is bright enough to be seen with the naked eye. Other articles where Mu Scorpii is discussed: star: Eclipsing binaries: …for the bright B-type star Mu Scorpii. μ¹ Scorpii; μ² Scorpii; They are separated by 0.1° in the sky. μ¹ Scorpii was member of asterism 尾 (Wěi), Tail and μ² Scorpii was stand alone in asterism 神宮 (Shén Gōng), Changing Room. The star is a eclipsing Beta Lyrae (Sheliak) variable type which means that its size changes over time. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. The source of the information if it has a Hip I.D. μ¹ Scorpii; μ² Scorpii; They are separated by 0.1° in the sky. A line through the Cat's Eyes points west (right) by nearly a fist-width toward Mu Scorpii, a much tighter pair known as the Little Cat's Eyes. Xamidimura is not part of the constellation outline but is within the borders of the constellation. Based on the spectral type, we can deduce that the surface temperature of the star is in the order of between between 10,000 and 25,000K based on the notes from Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The description is based on the spectral class. The figure is derived at by using the formula from Xamidimura has an apparent magnitude of 3.00 which is how bright we see the star from Earth. The time it will take to travel to this star is dependent on how fast you are going. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: . NGC 6281 is an open cluster of stars in the constellation Scorpius.It was not included in the Messier or Caldwell catalogues of nebulous objects, but it is the brightest such cluster in the constellation to be left out of both. an offensive content(racist, pornographic, injurious, etc.) If you want that in miles, it is about 3,038,661,455,398,608.01, based on 1 Ly = 5,878,625,373,183.61 miles.In 2007, Hipparcos data was revised with a new parallax of 6.88000 which put Pipirima at a distance of 474.07 light years or 145.35 parsecs. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. The star's Galacto-Centric Distance is 7,255.00 Parsecs or 23,663.15 Light Years. When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Comments may be merged or altered slightly such as if an email address is given in the main body of the comment.You can decline to give a name which if that is the case, the comment will be attributed to a random star. It is purely that the distance was recalculated. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).The source of the information if it has a Hip I.D. Proper Motion details the movements of these stars and are measured in milliarcseconds. Keep reading for comprehensive facts and information.
Primary / Proper / Traditional Name: Pipirima: Alternative Names: Mu2 Scorpii, Mu.02 Sco, HD 151985, HIP 82545, HR 6252: Spectral Type: B2IV: Constellation's Main Star
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