BETA (β) SCORPII
OPTICAL DOUBLE STAR
Right Ascension:
16h 05m 26.3s
Best Seen:
7/1 - 9/1
Declination:
-19º 48' 13"
Combined
Magnitude:
2.44
Computer File:
betasco
Constellation:
Scorpius
Apparent
Separation:
12.8"
Actual
Compared to Sun
Distance
530 / 1132 l.y
--
Actual Brightness
--
1970 / 1040
Magnitude
2.56 / 4.90
--
Mass
--
--
Surface Gravity
--
--
Surface Composition (by mass)
74% hydrogen 24% helium 2% everything else
same
Spectral Type
B0.5 V / B2 V
G2 V
Density (gram/cubic cm)
--
--
WHAT TO LOOK FOR THROUGH THE TELESCOPE:
-
Recommended eyepiece: 24mm or 40 mm.
-
When people look through the telescope they should see two stars next to each other. One star should be slightly brighter than the other.
-
INCLUDE THIS? Both stars have dimmer companion stars. They may be seen.
BETA SCORPII INFORMATION:
- The brighter star, Star A, is actually a multiple star.
a. However, we can’t see its companion: Star A is a “spectroscopic binary,” which means its companion is detected by looking at a spectra of Star A.
b. This companion is so close to Star A, they orbit each other in just under 7 days. This means they’re closer than Mercury is to our Sun.
-
The dimmer star, Star B, may also be part of a multiple system.
-
Through the telescope, dim stars can be seen close to both Stars A and B. It is unclear whether these stars form multiple systems with A and B, or if they are also optical doubles.
In here previously, but cannot be – this is an optical double, not a multiple:
- This is actually a 5-member system. A third star has a magnitude of 9.5 and a period of about 1,000 years.
Item
Updated
Notes
Coordinates
11-27-2002
difference between two, SIMBAD and Scott’s The Flamsteed Collection
Combined Magnitude
11-27-2002
with Flamsteed
Apparent Separation
11-27-2002
with Flamsteed
Distance
11-27-2002
with Flamsteed and SIMBAD
Actual Brightness
11-27-2002
with Flamsteed
Magnitude
11-27-2002
with Flamsteed
Mass
Surface Gravity
Surface Composition
01-06-2003
OK for all stars
Spectral Type
11-27-2002
with Flamsteed and SIMBAD
Density
Other Information
11-27-2002
from http://skyandtelescope.com/news/current/article_801_1.asp and SIMBAD
** NOTE: SIMBAD says Star A (HD 144217) is a “spectroscopic binary” while B (HD 144218) is a “Star in double system”