V354 Cephei

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 V354 Cephei, the location is 22h 33m 34.6 and 58° 53` 47.05 .

Physical Properties

Colour

Based on the star's spectral type of M2.5 Iab , V354 Cephei's colour and type is red supergiant star. Based on the spectral type, we can deduce that the surface temperature of the star is in the order of between below 3,500K 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

V354 Cephei Radius has been calculated as being 1,520.00 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,057,616,000.00.km. If you need the diameter of the star, you just need to multiple the radius by 2.

Apparent (Brightness) and Absolute Magnitudes

V354 Cephei has an apparent magnitude of 10.82, this is a measure of the brightness of the star as seen from Earth. Apparent Magnitude is also known as Visual Magnitude.

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.

Alternative Names and Meanings

Distance to V354 Cephei

V354 Cephei is an estimated 9,000.00 light years from our Solar System (Earth and Sun). It would take a spaceship 9,000.00 years travelling at the speed of light to get there. We don't have a space ship that can travel that distance or at that speed yet.

Comparison Between V354 Cephei 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 V354 Cephei 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 NameV354 CepheiThe Sun
Alternative NamesV354 CepSol
Spectral TypeM2.5 IabG2V
Star Type based on Spectral TypeSupergiant StarMain Sequence Star
ColourRedYellow (Atmosphere) / White (In Space)
GalaxyMilky WayMilky Way
ConstellationCepheusN/A
Constellation's Main StarNoN/A
Visual / Apparent Magnitude10.82-26.74
Naked Eye VisibleRequires a 4.5 - 6 Inch TelescopeYes (But don't look at it)
Right Ascension (R.A.)22h 33m 34.6N/A
Declination (Dec.)58° 53` 47.05N/A
Distance from the Sun / Earth9,000.00 Light Years
Radius1,520.000 1

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware8 (9 inc. Pluto)
Sun FactsSource

Cepheus's 5 Brightest Stars


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