Red supergiant field guide

Betelgeuse is a nearby laboratory for massive-star death.

Betelgeuse is the red shoulder star of Orion and one of the best naked-eye examples of a massive star near the end of its life. Its size, cool surface, convection, dust, and irregular brightness changes make it a practical study object for late-stage stellar evolution.

Betelgeuse extended atmosphere

Catalog identity

Observed properties

Aliases
Alpha Orionis
Constellation
Orion
Object class
Red supergiant variable star
Spectral class
M-type red supergiant, commonly listed near M1-M2 Ia-ab
Coordinates
RA 05h 55m 10.3s, Dec +07 deg 24 min 25 sec (J2000)
Distance
about 550 light-years (about 170 parsecs)
Visual brightness
variable, roughly magnitude 0.0 to 1.6 in visual light
Absolute magnitude
roughly -5 to -6 visual, depending on adopted distance and state

Physical scale

Why it is extreme

Mass
about 16 to 20 solar masses; model dependent
Radius
roughly 700 to 900 solar radii; variable and model dependent
Solar-system scale
if placed at the Sun, its outer atmosphere would reach near the inner asteroid belt scale
Temperature
about 3,500 K effective temperature
Luminosity
order of 100,000 solar luminosities
Variability
semi-regular pulsation, giant convection cells, dust episodes, and long secondary variability
Great dimming
2019-2020 fading was consistent with surface cooling plus dust/mass-loss effects
Future state
expected to end as a core-collapse supernova on astronomical timescales, but not predictably soon for human scheduling

Physics Themes

What Betelgeuse teaches

Red supergiant structure

The outer envelope is cool, extended, and convective. A clean solid surface is the wrong mental model; the visible photosphere and atmosphere are dynamic layers.

Mass loss

Dust formation, stellar wind, and episodic ejections remove material before core collapse, shaping the eventual circumstellar environment.

Variable brightness

Betelgeuse changes brightness because pulsation, convection, temperature patches, and dust along the line of sight all affect visible light.

Supernova caution

It is a credible future supernova progenitor, but no current observation lets a website predict a human-calendar explosion date.

Angular resolution

Its large apparent diameter makes it one of the few stars where interferometry can probe surface structure rather than only integrated light.

Scale discipline

A red supergiant radius is enormous compared with planets, but its distance is measured in hundreds of light-years, so it belongs in the deep-space layer.

Simulator interpretation

What the 3D view shows

The 3D simulator places Betelgeuse in the light-year deep-space context, not inside the AU-scale solar-system map. The marker uses a red supergiant glow, an extended atmosphere shell, and mass-loss plumes as a readable study model.

Research workflow

How to study it

Use SkyMap for Orion field placement, then compare visual light curves, infrared dust emission, spectroscopy, and interferometric diameter work. Treat radius, distance, and luminosity values as model-dependent ranges, not single exact constants.

Mathematical model

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