HR2290 is a main-sequence star in the constellation of Puppis.
HR2290 visual magnitude is 6.6. Because of its reltive faintness, HR2290 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR2290:
Celestial coordinates and finder chart of HR2290
HR2290 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2290 are provided in the following table:
The simplified sky map below shows the position of HR2290 in the sky:
Visibility of HR2290 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR2290 is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of HR2290
The image below is a photograph of HR2290 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of HR2290 is 0.231 arcsec per year in Right Ascension and -0.271 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR2290 from the Sun and relative movement
HR2290 is distant 83.76 light years from the Sun and it is moving far from the Sun at the speed of 60 kilometers per second.
Spectral properties of HR2290
HR2290 belongs to spectral class G3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2290 is situated in the Hertzsprung–Russell diagram.