Menu

QR Vulpeculae — Double Star in Vulpecula

DoubleStar Vulpecula (Vul) Visible
Star Map
+ List + Plan

Observe

1Physical Properties

Magnitude 4.78
Range 4.60 - 4.81
Variable Type Gamma Cassiopeiae (Eruptive Be Star)
Spectral Type B3Ve
Star Color Blue (B-V -0.18)

2Position & Identifiers

RA 20h 15m 15.9s
Dec +25° 35' 31.0"
Constellation Vulpecula (Vul)
HR 7739
HIP 99824
HD 192685
Variable ID QR Vul
Double Cat 13589

3How easy to split?

Primary 4.8 mag Companion 7.6 mag Separation 0.4″
Sign in and configure your equipment and default location to see a personalized row.
Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. V. hard V. hard V. hard
C8 203mm V. hard V. hard V. hard
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 760 mm reflector.

4Visibility

Set a location in User Settings to see visibility data.

Best season Jun – Aug (peak: Jul)

5Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 0.4″
Companion Mag 7.5
Position Angle 190°
Star Colors A: Blue B: Yellow-white
Discoverer BU 983
AB CPM, 680?y.

Separation over time

Measured 1879 → 2016 (137 y)
Separation drift 0.80" → 0.40" (-0.40")
Rate -0.0029" / y
PA drift 154° → 190° (+36°, +0.263°/y)

Essentially fixed on human timescales — the same view your grandchildren will see.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

Log in to set your own equipment
80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 190°

A: 4.8 · B: 7.5 · Sep: 0.4″ · PA: 190° · N up, E left

Unresolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

6

Size Comparison

Querying VizieR for stellar data…
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

4.60 - 4.80V. Sudden brightening in 1982, amp. 0.18V.
11.000d, subsequently rejected; probably shorter if variable.
Discovered in 1982 as a Be star. H alpha previously absorption; emission increased rapidly in September 1982.

Survey Image

Loading survey image…

}