Your guide to the Solar System and the night sky
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🌎  Observing from: Greenwich, United Kingdom [change]

ω Draconis (omega Draconis)

ω Draconis is a double main-sequence star in the constellation of Draco.

ω Draconis visual magnitude is 4.8. Because of its moderate brightness, ω Draconis should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.

The table below summarizes the key facts about ω Draconis:

4.8
Main-sequence
ω Draconis (omega Draconis) is above the horizon from Greenwich, United Kingdom [change]. Altitude: 31°.

Celestial coordinates and finder chart of ω Draconis

ω Draconis is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of ω Draconis are provided in the following table:

17h 36m 57s
+68° 45’ 29”
99.08°
31.87°
Draco

The simplified sky map below shows the position of ω Draconis in the sky:

Finder chart ω Draconis (omega Draconis) star
Simplified finder chart for ω Draconis (omega Draconis).

Visibility of ω Draconis from your location

Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London

ω Draconis (omega Draconis) is circumpolar and transits at 08:28 UTC (altitude: 72.7°)

Digitized Sky Survey image of ω Draconis

The image below is a photograph of ω Draconis 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 ω Draconis is 0.002 arcsec per year in Right Ascension and 0.323 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Image of ω Draconis (omega Draconis) star
DSS2 image of ω Draconis. The red arrow shows the motion of ω Draconis during the next 1000 years (0.03 arcmin in Right Ascension and 5.38 arcmin in declination);

Distance of ω Draconis from the Sun and relative movement

ω Draconis is distant 76.49 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.

23.46 pc
76.49 ly
-14 km/s
0.002 arcsec/year
0.323 arcsec/year

Spectral properties of ω Draconis

ω Draconis belongs to spectral class F5 and has a luminosity class of V corresponding to a main-sequence star.

2.95
F5V
6724K

The red dot in the diagram below shows where ω Draconis is situated in the Hertzsprung–Russell diagram.

HR Diagram
H-R diagram showing the position of ω Draconis. Attribution: Richard Powell / CC BY-SA

ω Draconis star system properties

ω Draconis 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 ω Draconis double sysyem:

4.8
13.1
8.3
72.3 arcsec

Alternative designations of ω Draconis

ω Draconis
(omega Draconis)
28 Draconis
SAO17576
SAO17576