Universe Guide
SearchTwitterComments

BF Sagittae (Carbon Star) Facts

BF Sagittae Facts

BF Sagittae's Alternative Names

HIP98662 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD190048.

BF Sagittae has alternative name(s) :- , BF Sge.

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+20 4390.

More details on objects' alternative names can be found at Star Names .

Location of BF Sagittae

The location of the Carbon star in the night sky 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 object is compared to the celestial equator and is expressed in degrees. For BF Sagittae, the location is 20h 02m 23.08 and +21° 05` 24.9 .

Radial Velocity and Proper Motion of BF Sagittae

Proper Motion

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 -5.43 ± 0.67 milliarcseconds/year towards the north and -1.17 ± 1.09 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -14.00 km/s with an error of about 3.20 km/s . 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. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

Physical Properties (Colour, Temperature) of BF Sagittae

BF Sagittae Colour and Temperature

BF Sagittae has a spectral type of C5II. This means the star is a carbon red Carbon star. The star has a B-V Colour Index of 1.6 which means the star's temperature is about 3,775 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu at being .

BF Sagittae Apparent and Absolute Magnitudes

BF Sagittae has an apparent magnitude of 9.14 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 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.26. 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 BF Sagittae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -0.01 which gave the calculated distance to BF Sagittae as -326163.34 light years away from Earth or -100000 parsecs. If you want that in miles, it is -218,730,559,574,181.

In 2007, Hipparcos data was revised with a new parallax of 1.32 which put BF Sagittae at a distance of 2470.93 light years or 757.58 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.

Using the 2007 distance, the star is roughly 156,261,003.07 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun.

Travel Time to BF Sagittae

The time it will take to travel to this star is dependent on how fast you are going. U.G. has done some calculations as to how long it will take going at differing speeds. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. Its primary mission was to visit Pluto which at the time of launch (2006), Pluto was still a planet.

DescriptionSpeed (m.p.h.)Time (years)
Walking4414,261,686,773.74
Car12013,808,722,892.46
Airbus A3807362,251,422,210.73
Speed of Sound (Mach 1)767.2692,159,668,573.99
Concorde (Mach 2)1,534.541,079,832,879.62
New Horizons Probe33,00050,213,537.79
Speed of Light670,616,629.002,470.93

Variable Type of BF Sagittae

The star is a pulsating Slow Irregular 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. BF Sagittae brightness ranges from a magnitude of 9.370 to a magnitude of 9.110 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.2 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.

Hide Explanations
Show GridLines

Additional BF Sagittae Facts and Figures

Visual Facts


Primary / Proper / Traditional NameBF Sagittae
Alternative NamesHD 190048, HIP 98662, BD+20 4390, BF Sge
Spectral TypeC5II
Constellation's Main StarNo
Multiple Star SystemYes
Star TypeCarbon Star
ColourRed
GalaxyMilky Way
ConstellationSagitta
Absolute Magnitude / -0.26
Visual / Apparent Magnitude9.14
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)20h 02m 23.08
Declination (Dec.)+21° 05` 24.9
Galactic Latitude-5.10 degrees
Galactic Longitude59.78 degrees
1997 Distance from Earth-0.01 Parallax (milliarcseconds)
 -326163.34 Light Years
 -100000 Parsecs
2007 Distance from Earth1.32 Parallax (milliarcseconds)
 2470.93 Light Years
  757.58 Parsecs
 156,261,003.07 Astronomical Units
Proper Motion Dec.-5.43 ± 0.67 milliarcseconds/year
Proper Motion RA.-1.17 ± 1.09 milliarcseconds/year
B-V Index1.60
Radial Velocity-14.00 ± 3.20 km/s

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassPulsating
Variable Star TypeSlow Irregular
Mean Variability Period in Days0.211
Variable Magnitude Range (Brighter - Dimmer)9.110 - 9.370

Estimated Calculated Facts


Effective Temperature3,775 Kelvin

Sources and Links


SIMBAD SourceLink

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
190048+20 4390.0A9.90000-1.00000-6.00000CI
B10.20000-1.00000-6.000001991

Related Stars


Comments and Questions

There's no register feature and no need to give an email address if you don't need to. All messages will be reviewed before being displayed. 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. A name is preferred even if its a random made up one by yourself.

   
x
This website is using cookies. More info. That's Fine