Universe Guide
AliensAliensConstellationsTelevision and Films ListFact ListGames ListWarcraftSearchTwitterFacebook


U Sagittae, HD181182, HIP94910, HR7326

U Sagittae is a blue eclipsing star that can be located in the constellation of Sagitta. The star can not be seen by the naked eye, you need a telescope to see it.

The Id of the star in the Yale Bright Star Catalogue is HR7326. HIP94910 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD181182.

U Sagittae has alternative name(s), U Sge.

Location of U Sagittae

The location of the star in the galaxy is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the star is compared to the celestial equator and is expressed in degrees. For U Sagittae, the location is 19h 18m 48.41 and +19d 36` 37.7 .

Proper Motion of U Sagittae

All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Proper Motion details the movements of these stars and are measured in milliarcseconds. The star is moving 1.06 ± 0.33 miliarcseconds/year towards the north and 1.02 ± 0.50 miliarcseconds/year east if we saw them in the horizon. The Radial Velocity, that is the speed at which the star is moving away/towards us is -10.10000 km/s with an error of about 7.40 km/s .

Physical Properties (Colour, Temperature, Radius) of U Sagittae

U Sagittae has a spectral type of B8III + K. This means the star is a blue star. The star is 7262.00000000 Parsecs from the Galactic Centre or terms of Light Years is 23685.9820412800000000s. The star has a B-V Colour Index of 0 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 9,531 Kelvin.

U Sagittae Radius has been calculated as being 5.33 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,707,834.29.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 4.12. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

U Sagittae Apparent and Absolute Magnitudes

U Sagittae has an apparent magnitude of 6.50 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of -0.96 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.40. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.

Distance to U Sagittae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 3.22 which gave the calculated distance to U Sagittae as 1012.93 light years away from Earth or 310.56 parsecs. It would take a spaceship travelling at the speed of light, 1012.93 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

In 2007, Hipparcos data was revised with a new parallax of 4.17 which put U Sagittae at a distance of 782.17 light years or 239.81 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.

The star's Galacto-Centric Distance is 7,262.00 Parsecs or 23,685.98 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Variable Type of U Sagittae

The star is a eclipsing Beta Persei (Algol)/Semi-Detached System (subtype) variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. U Sagittae brightness ranges from a magnitude of 9.100 to a magnitude of 6.498 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 3.4 days (variability).

Source of Information

The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

U Sagittae Facts

Alternative Names

Traditional/Proper NameU Sagittae
Short NameU Sge
Hipparcos Library I.D.94910
Yale Bright Star Catalogue (HR) Id7326
Bonner DurchmusterungBD+19 3975
Henry Draper Designation181182

Visual Facts

Star Type star
Absolute Magnitude-0.96 / -0.40
Visual / Apparent Magnitude6.50
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)19h 18m 48.41
Declination (Dec.)+19d 36` 37.7
Galactic Latitude3.05 degrees
Galactic Longitude53.44 degrees
1997 Distance from Earth3.22 Parallax (milliarcseconds)
 1012.93 Light Years
 310.56 Parsecs
2007 Revised Distance from Earth4.17 Parallax (milliarcseconds)
 782.17 Light Years
 239.81 Parsecs
Galacto-Centric Distance23,685.98 Light Years / 7,262.00 Parsecs
Proper Motion Dec.1.06 ± 0.33 milliarcseconds/year
Proper Motion RA.1.02 ± 0.50 milliarcseconds/year
B-V Index0.00
Radial Velocity-10.10 ± 7.40 km/s
Spectral TypeB8III + K
Colour(B) blue

Variable Star Details

Variable Star ClassEclipsing
Variable Star TypeBeta Persei (Algol)/Semi-Detached System (subtype)
Mean Variability Period in Days3.381
Variable Magnitude Range (Brighter - Dimmer)6.498 - 9.100

Estimated Facts

Calculated Effective Temperature9,531 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Multi-Star System

The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.

Proper Motion mas/yr
H.D. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
181182+19 3975.0A9.0000018.00000B9Blue/White
231125+19 3974.0B9.500009.0000016.00000G5Yellow1875

Add a Comment

Email: (Optional)