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Theta Scorpii

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Also known as Sargas

star in the southern zodiac constellation of Scorpius

Astronomical data · SIMBAD

Object type
*
Spectral type
F1III
Distance
300 light-years
Redshift
z = 0.00001727876940926798
Coordinates
RA 264.3297° · Dec -42.9978°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Constellation
Scorpius
Right ascension
17 37 19.12985
Declination
−42 ° 59 ′ 52.1808 ″
Apparent magnitude v
1.84 (1.862 + 6.22)
Evolutionary stage
Post- stellar merger
Spectral type
F1III
U b color index
+0.21
B v color index
+0.40

via Wikipedia infobox

Wikidata facts

Instance of
binary star
Constellation
Scorpius
Distance from Earth
270
Radius
20
Mass
3.7
Image
Scorpius constellation map.png
Show 12 more facts
stellar rotational velocity
125
catalog code
TD1 20659
spectral class
F0
luminosity
960
parallax
10.86
apparent magnitude
0.841
right ascension
264.329707721
declination
-42.997827993
radial velocity
5.0
epoch
J2000.0
right ascension component of proper motion
19
declination component of proper motion
6
Sources (1)

via Wikidata · CC0

~3 min read

Encyclopedic overview

Theta Scorpii (θ Scorpii, abbreviated Theta Sco, θ Sco) is a binary star in the southern zodiac constellation of Scorpius. The apparent visual magnitude of this star is +1.87, making it readily visible to the naked eye and one of the brightest stars in the night sky. It is sufficiently near that the distance can be measured directly using the parallax technique and such measurements obtained during the Hipparcos mission yield an estimate of approximately 329 light-years (101 parsecs) from the Sun.

The two components are designated θ Scorpii A (officially named Sargas /ˈsɑːrɡæs/, the traditional name for the system) and B.

Excerpted from Wikipedia’s “Theta Scorpii” article, available under the CC BY-SA 4.0 licence.