Menu

V856 Scorpii — Variable Star in Scorpius

Observable Variable Star Good (57/100)

Range: 6.64 - 8.44, Period: 30.0d, Type: UXOR

Magnitude 7.0–7.7m VariableStar Scorpius (Sco) Visible
Star Map
+ List + Plan Star Hop

Observe

1Physical Properties

Magnitude 7.05
Range 6.64 - 8.44
Variable Type UXOR
Spectral Type A7IVe supergiant
Star Color Yellow-white (B-V 0.36)

2Position & Identifiers

RA 16h 08m 34.2s
Dec -39° 06' 19.0"
Constellation Scorpius (Sco)
HR 5999
HIP 79080
HD 144668
SAO 207367
Variable ID V856 Sco

3How easy to follow?

Magnitude 7.0 – 7.7 mag Amplitude 0.7 mag Period 30 d Type UXOR
Sign in and configure your equipment and default location to see a personalized row.
Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Imp. Imp. Imp.
50mm finder Medium Medium Hard+
150mm scope Medium Medium Medium
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

Set a location in User Settings to see visibility data.

Best season Apr – Jun (peak: May)

5Survey Image

Loading survey image…

6Comparison Stars

Nearby stable stars for estimating brightness (AAVSO)

Loading comparison stars…

Explore

7

Size Comparison

Querying VizieR for stellar data…
8

Compare Stars

9

Spectral Classification

10

Hertzsprung-Russell Diagram

Loading HR diagram…
11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

14

Stellar Fusion

Discover

15Stellar Notes

6.97 - 7.71V, about 30d, variability attributed to circumstellar dust. Possibly a binary shell star with mass exchange. | Considerable confusion between HR 5999 and 6000 particularly as to which is the variable and which the brighter. | Originally announced as HR 6000, V856 Sco is really HR 5999, the southern preceding and fainter component C of the | bright double. The error stems from interchanged photometric data in Harvard Annals 45, 197, 1901, all other early | visual and photographic estimates indicating that the S. prec. component is the fainter.
CPM with HR 6000 at 44". CD, 7.1, 11.7v, sep. 1.3".
}