δ Antliae (delta Antliae)
δ Antliae is a variable and double main-sequence star in the constellation of Antlia.
δ Antliae visual magnitude is 5.56. Because of its reltive faintness, δ Antliae 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 δ Antliae:
Celestial coordinates and finder chart of δ Antliae
δ Antliae is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of δ Antliae are provided in the following table:
The simplified sky map below shows the position of δ Antliae in the sky:
Visibility of δ Antliae from your location
Digitized Sky Survey image of δ Antliae
The image below is a photograph of δ Antliae 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 δ Antliae is -0.033 arcsec per year in Right Ascension and 0 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of δ Antliae from the Sun and relative movement
δ Antliae is distant 480.83 light years from the Sun and it is moving far from the Sun at the speed of 14 kilometers per second.
Spectral properties of δ Antliae
δ Antliae belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where δ Antliae is situated in the Hertzsprung–Russell diagram.
δ Antliae star system properties
δ Antliae is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the δ Antliae double sysyem: