HR4183
HR4183 is a double giant star in the constellation of Antlia.
HR4183 visual magnitude is 6.37. Because of its reltive faintness, HR4183 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 HR4183:
Celestial coordinates and finder chart of HR4183
HR4183 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 HR4183 are provided in the following table:
The simplified sky map below shows the position of HR4183 in the sky:

Visibility of HR4183 from your location
Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR4183 rise, transit and set times from Greenwich, United Kingdom [change] are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR4183
The image below is a photograph of HR4183 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 HR4183 is -0.021 arcsec per year in Right Ascension and 0.001 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR4183 from the Sun and relative movement
HR4183 is distant 695.10 light years from the Sun and it is moving far from the Sun at the speed of 11 kilometers per second.
Spectral properties of HR4183
HR4183 belongs to spectral class G8 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR4183 is situated in the Hertzsprung–Russell diagram.

HR4183 star system properties
HR4183 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR4183 double sysyem: