Menu

Deneb

HIP 102098; Alpha Cygni; 50 Cygni

HIP 102098; Alpha Cyg; 50 Cyg DoubleStar Cygnus (Cyg) Visible
Star Map
+ List + Plan Back

About Deneb

Description

Deneb is a blue-white supergiant of spectral type A2Ia at magnitude 1.25, the brightest star in Cygnus and one of the most luminous stars visible to the naked eye. Its distance is uncertain but estimated at 1,500-2,600 light-years, making its intrinsic luminosity between 55,000 and 196,000 times solar. Deneb is evolving toward becoming a red supergiant and will eventually explode as a supernova.

Observing Tips

Deneb marks the top of the Northern Cross asterism in Cygnus and is the faintest vertex of the Summer Triangle (with Vega and Altair). Despite appearing dimmer than Vega and Altair, it is vastly more luminous — just much farther away. Its location in the Milky Way makes the surrounding field spectacular in binoculars. Best observed June through November.

History

The name Deneb comes from the Arabic 'dhanab al-dajajah,' meaning 'the tail of the hen.' As the prototype A-type supergiant, Deneb has been extensively studied. It will become the pole star (roughly) around AD 9800 as Earth's axis precesses. In Chinese astronomy, Deneb represents a bridge across the Milky Way.

Fun Facts

If Deneb were at the same distance as Sirius (8.6 light-years), it would be roughly as bright as a half Moon and would cast visible shadows at night. Its exact distance remains one of the most debated values in stellar astronomy — Hipparcos measurements have large error bars for such a distant star.

Observe

1Physical Properties

Magnitude 1.25
Range 1.21 - 1.29
Variable Type ACYG
Spectral Type A2Ia
Star Color White (B-V 0.09)
Temperature 8519 K
Radius 203.0 R☉
Distance 1,380 ly

Position & Identifiers

RA 20h 41m 25.9s
Dec +45° 16' 49.0"
Constellation Cygnus (Cyg)
HR 7924
HIP 102098
HD 197345
Bayer Alpha
Flamsteed 50 Cyg
Variable ID Alp Cyg
Double Cat 14172

2How easy to split?

Primary 1.3 mag Companion 11.7 mag Separation 75.6″
Sign in and configure your equipment and default location to see a personalized row.
Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard V. hard+ V. hard
150mm Newt. Medium Hard+ Hard
C8 203mm Medium+ Medium Medium
Easy Medium Hard Very hard Impossible

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

3Visibility

Set a location in User Settings to see visibility data.

Best season Jun – Aug (peak: Jul)

4Multiple Star System

Separation 75.6″
Companion Mag 11.7
Position Angle 105°
Star Colors A: White
Discoverer H N 73

Eyepiece View

Log in to set your own equipment
80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 105°

A: 1.2 · B: 11.7 · Sep: 75.6″ · PA: 105° · N up, E left

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

Explore

6

Size Comparison

7

Compare Stars

8

Stellar Lifecycle

9

Spectral Classification

10

Hertzsprung-Russell Diagram

Loading HR diagram…
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

Alpha Cyg 1.21 - 1.29V. Change in H:H epsilon. No emission recorded before 1944.
The following two orbits are reported as equally probable: 846.8d, K 3.12k/s, V0 -2.81k/s; 776.4d, K 2.61k/s, | V0 -3.24k/s.
Cyg OB7.
Mass loss 3x10E-10 solar masses/y.
DENEB; Deneb Cygni; Deneb el Adige; Arided; Aridif; Gallina; Arrioph.
15

Light Travel Time Machine

16

Relativistic Travel

Survey Image

Loading survey image…

}