Universe Guide

HD 300034

HD 300034 Facts

  • HD 300034 is a star that can be located in the constellation of Vela. The description is based on the spectral class.
  • HD 300034 is not part of the constellation outline but is within the borders of the constellation.
  • Based on the spectral type (A5 E) of the star, the star's colour is blue - white .
  • The star is calculated at being about 3657.77 light years away from us. Distance

HD 300034's Alternative Names

The Id of the star in the Henry Draper catalogue is HD300034.

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

Location of HD 300034

The location of the 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 HD 300034, the location is 09 25 23.3201322252 and -55 23 02.257502772 .

Proper Motion of HD 300034

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 5.59 milliarcseconds/year towards the north and -8.57 milliarcseconds/year east if we saw them in the horizon. . 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 of HD 300034

HD 300034 Temperature and Colour

Based on the star's spectral type of A5 E , HD 300034's colour and type is blue - white star. Based on the star's spectral, the stars temperature is between 7,500.00 and 10,000.00 degrees kelvin.

Distance to HD 300034

The Parallax of the star is given as 0.89170 which gives a calculated distance to HD 300034 of 3657.77 light years from the Earth or 1121.45 parsecs. It is about 21,502,659,531,269,813 miles from Earth.

The star is roughly 231,314,055.15 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 HD 300034

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)
Airbus A3807363,332,827,971.55
Speed of Sound (Mach 1)767.2693,197,003,120.23
Concorde (Mach 2)1,534.541,598,499,476.75
New Horizons Probe33,00074,332,163.24
Speed of Light670,616,629.003,657.77

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Additional HD 300034 Facts and Figures

Visual Facts

Primary / Proper / Traditional NameHD 300034
Alternative NamesHD 300034
Spectral TypeA5 E
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeStar
GalaxyMilky Way
Right Ascension (R.A.)09 25 23.3201322252
Declination (Dec.)-55 23 02.257502772
Distance from Earth0.89170 Parallax (milliarcseconds)
 3657.77 Light Years
 1121.45 Parsecs
 231,314,055.15 Astronomical Units
Proper Motion Dec.5.58800 milliarcseconds/year
Proper Motion RA.-8.57100 milliarcseconds/year

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Estimated Calculated Facts

Calculated Temperature Range7,500.00 - 10,000.00

Sources and Links


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