39 Andromedae
39 Andromedae is a double star in the constellation of Andromeda.
39 Andromedae visual magnitude is 5.98. Because of its reltive faintness, 39 Andromedae 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 39 Andromedae:
Celestial coordinates and finder chart of 39 Andromedae
39 Andromedae is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 39 Andromedae are provided in the following table:
The simplified sky map below shows the position of 39 Andromedae in the sky:
Visibility of 39 Andromedae from your location
Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
39 Andromedae is circumpolar and transits at 06:21 UTC (altitude: 79.9°)
Digitized Sky Survey image of 39 Andromedae
The image below is a photograph of 39 Andromedae 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 39 Andromedae is -0.02 arcsec per year in Right Ascension and -0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 39 Andromedae from the Sun and relative movement
39 Andromedae is distant 343.52 light years from the Sun and it is moving far from the Sun at the speed of 4 kilometers per second.
Spectral properties of 39 Andromedae
39 Andromedae belongs to spectral class A5
The red dot in the diagram below shows where 39 Andromedae is situated in the Hertzsprung–Russell diagram.
39 Andromedae star system properties
39 Andromedae is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the 39 Andromedae double sysyem: