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Temperature

Neutron star surface

Neutron star surface temperature is the intense heat found at the outer layer of a young neutron star after a supernova.

Also known as: neutron star surface temperature

How big is it?

1,000,000 K · representative young surface temperature

Representative young surface temperature · representative
Typical recorded range: 100,000 K to 10,000,000 K.

Scale illustration of a neutron star’s surface, showing the recorded representative young surface temperature.
Recorded representative young surface temperature: 1,000,000 K.

A little perspective

Neutron star surface vs Fusion plasma: temperature comparison

The young surface temperature of a neutron star’s surface is 99,000,000 K lower than the temperature of fusion plasma.

Scale
Neutron star surface

Neutron star surface temperature is the intense heat found at the outer layer of a young neutron star after a supernova.

1,000,000 KRepresentative young surface temperature
0 K · absolute zero
Fusion plasma

Fusion plasma is a state of matter where atomic nuclei and electrons are separated and nuclei can undergo nuclear fusion.

100,000,000 KTemperature
0 K · absolute zero
Celsius and Fahrenheit zero points are offsets. Compare temperature differences, not ratios in °C or °F. The kelvin axis starts at absolute zero.
Measurements, assumptions & sources +

Neutron star surface

Representative young surface temperature: 1,000,000 K; representative; range 100,000 K–10,000,000 K.

A representative one-million-kelvin thermal surface scale for a young neutron star. Surface temperature falls as the remnant cools and depends on age, magnetic field, atmosphere and observing model.

NASA Imagine the Universe — Neutron stars

The marked representative young surface temperature is calibrated. Unmeasured illustration details are representative.

Fusion plasma

Temperature: 100,000,000 K; defined reference.

A 100 million K plasma example. High temperature alone does not specify total thermal energy.

Defined examples — our methodology

The marked temperature is calibrated. Unmeasured illustration details are representative.

Use the visual comparison to explore its scale, then check the measurements and sources.

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Why this measurement?

Why we use 1,000,000 K

We compare the young surface temperature of a neutron star’s surface. This is a representative comparison value; individual specimens or conditions can vary. The recorded range is 100,000 K to 10,000,000 K.

A representative one-million-kelvin thermal surface scale for a young neutron star. Surface temperature falls as the remnant cools and depends on age, magnetic field, atmosphere and observing model.

The picture identifies the subject; the diagram compares the recorded values. How calibrated comparisons work →

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Recorded properties

Dimensions and measurements

PropertySelected valueRecorded rangeBasis
1,000,000 K100,000 K to 10,000,000 Krepresentative

Around this scale

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Sources and method

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The source records and measurement method remain available for inspection.

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