Rho Cassiopeiae (7 Cassiopeiae) Star Facts

Facts

Location

The location of the supergiant 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 Rho Cassiopeiae, the location is 23h 54m 23.04 and +57° 29` 57.8 .

Radial Velocity and Proper Motion

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 -3.73 ± 0.15 milliarcseconds/year towards the north and -4.48 ± 0.21 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 -54.30000 km/s with an error of about 0.40 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 and Temperature

Based on the star's spectral type of F8Iavar , Rho Cassiopeiae's colour and type is yellow to white supergiant star. Based on the spectral type, we can deduce that the surface temperature of the star is in the order of between 6,000 and 7,500K based on the notes from Harvard University. To put this in context, the temperature of our Sun is about 5,778 Kelvin as said by Google.

Radius

Rho Cassiopeiae estimated radius has been calculated as being 660.87 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 459,833,623.43.km. If you need the diameter of the star, you just need to multiple the radius by 2. The figure is derived at by using the formula from SDSS rather than peer reviewed papers. It has been known to produce widely incorrect figures.

Rho Cassiopeiae Iron Abundance

Rho Cassiopeiae Iron Abundance is 0.05 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.

Apparent (Brightness) and Absolute Magnitudes

Rho Cassiopeiae has an apparent magnitude of 4.51, this is a measure of the brightness of the star as seen from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of -8.25

Absolute Magnitude is the apparent magnitude of the star from a distance of 10 parsecs or 32.6 light years. This assumes that there is nothing in between the object and the viewer such as dust clouds. To really compare the brightness of the star, it is best to use Absolute rather than Apparent Magnitude.

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 from Earth

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 0.28000 which gave the calculated distance to Rho Cassiopeiae as 11648.69 light years away from Earth or 3571.43 parsecs. If you want that in miles, it is about 68,478,284,598,350,185.97, based on 1 Ly = 5,878,625,373,183.61 miles.

Alternative Names and Meanings

Travel Time

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.

Mach 1 is the speed of sound, Mach 2 is twice the speed of sound. Corncorde before it was retired was the fastest commercial airline across the Atlantic and only one that could do Mach 2.

DescriptionSpeed (m.p.h.)Time (years)
Walking41,952,951,305,016.50
Car12065,098,376,833.88
Airbus A38073610,613,865,788.13
Mach 1767.26910,181,312,186.56
Mach 21,534.545,090,649,458.51
New Horizons33,000236,721,370.31
Speed of Light670,616,629.0011,648.69
Rho Cassiopeiae brightness ranges from a magnitude of 4.755 to a magnitude of 4.574 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.

Comparison Between Rho Cassiopeiae and The Sun

Below is a tabular view of the star facts with the values of the Sun on the right so you can compare against our own star, the Sun. The Sun is our nearest star and it is what keeps us warm and gives us light as we complete one orbit in 365.24 days.

If you want to see the comparison between Rho Cassiopeiae and our star, the Sun, you will need a screen of at least 800px across. Rotating your screen maybe sufficient to see the Stellar values for comparison.

Visual Facts


Primary NameRho CassiopeiaeThe Sun
Alternative NamesRho Cas, HD 224014, TycId 4009-2605-1, HIP 117863, HR 9045, 7 Cassiopeiae, 7 Cas, BD +56 3111, rho CasSol
Spectral TypeF8IavarG2V
Star Type based on Spectral TypeSupergiant StarMain Sequence Star
Colour Yellow - WhiteYellow (Atmosphere) / White (In Space)
GalaxyMilky WayMilky Way
ConstellationCassiopeiaN/A
Constellation's Main StarNoN/A
Absolute Magnitude -8.25 .38
Visual / Apparent Magnitude4.51-26.74
Naked Eye VisibleYesYes (But don't look at it)
Right Ascension (R.A.)23h 54m 23.04N/A
Declination (Dec.)+57° 29` 57.8N/A
Galactic Latitude-4.52456868 °
Galactic Longitude115.30068442 °
Distance from Earth0.28000 Parallax (milliarcseconds)N/A
 11648.69 Light Years8 Lt. Mins, 20 Lt. Sec.
 3571.43 Parsecs0.0000049264 A.U.
 736,655,183.89 Astronomical Units1
Proper Motion Dec.-3.73000 ± 0.15000 milliarcseconds/yearN/A
Proper Motion RA.-4.48000 ± 0.21000 milliarcseconds/yearN/A
B-V Index1.190.656 +/- 0.005
Radial Velocity-54.30000 ± 0.40 km/s-
Iron Abundance (Fe/H)0.0500 ± 9.990.14
Effective Temperature (Kelvin) 4586 5,772

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware8 (9 inc. Pluto)

Variable Star Details


Variable Star Class-
Variable Star TypeLong Period Variable-
Mean Variability Period in Days0.1724,015 (11 Years)
Variable Magnitude Range (Brighter - Dimmer)4.574 - 4.755-

Estimated Calculated Facts


Radius (x the Sun)660.87 / 0.00 1
Surface Temperature between 6,000 and 7,500K 5,778K

Sources and Links


SIMBAD SourceLink
Sun FactsSource

Map of Rho Cassiopeiae's Location in Cassiopeia


Map of Rho Cassiopeiae Location in Cassiopeia)

The map was generated using Night Vision, an awesome free application by Brian Simpson.

Cassiopeia's 5 Brightest Stars


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