Menu

HIP 82706 — Star in Scorpius

Wolf-Rayet

Late-stage massive star with a dense stellar wind; radius is taken from published spectral models rather than estimated from spectral class.

Read: Wolf-Rayet Stars — The Shortest, Fiercest Lives in the Galaxy
Magnitude 6.6m Star Scorpius (Sco) Visible
Star Map
+ List + Plan Star Hop

Observe

1Physical Properties

Magnitude 6.59
Spectral Type WC7+O5-8 Wolf-Rayet
Late-stage massive star with a dense stellar wind; radius is taken from published spectral models rather than estimated from spectral class.
Star Color Blue (B-V 0.21) (reddened by dust)
Radius 3.5 R☉

2Position & Identifiers

RA 16h 54m 19.6s
Dec -41° 49' 12.0"
Constellation Scorpius (Sco)
HR 6265
HIP 82706
HD 152270
SAO 227390
Variable ID Var?

3How easy to spot?

Sign in and configure your equipment and default location to see a personalized row.
Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Hard V. hard+ V. hard
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
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…

Explore

6

Size Comparison

7

Compare Stars

8

Spectral Classification

9

Hertzsprung-Russell Diagram

Loading HR diagram…
10

Stellar Lifecycle

11

Blackbody Spectrum

12

Stellar Absorption Spectrum

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

13

Stellar Fusion

Discover

14Stellar Notes

Innes and IDS data on components and number of components appear inconsistent. Probably different cluster components | measured.
Component A of visual double, 8.893d, K 142k/s, V0 -27.2k/s, msin3i 1.75, asini 17.4. Same period for both | absorption and emission lines, but differ in phase by 0.5 period.
Strongly reddened.
In cluster NGC 6231 #220. See HR 6260.
Shell of WR component expanding at 1688k/s.
}