Celestial hemisphere:  Northern  ·  Constellation: Taurus (Tau)  ·  Contains:  M 1  ·  NGC 1952
Getting plate-solving status, please wait...
M1 The Crab Nebula, Prodromos
M1 The Crab Nebula
Powered byPixInsight

M1 The Crab Nebula

Getting plate-solving status, please wait...
M1 The Crab Nebula, Prodromos
M1 The Crab Nebula
Powered byPixInsight

M1 The Crab Nebula

Equipment

Loading...

Acquisition details

Loading...

Description

The Crab Nebula, designated as Messier 1 (M1), is a supernova remnant located in the constellation Taurus. It is the result of a supernova explosion observed by Chinese astronomers in the year 1054. The remnant is situated approximately 6,500 light-years away from Earth and spans about 11 light-years in diameter. The Crab Nebula is characterized by its pulsar, a rapidly rotating neutron star formed during the supernova event. This pulsar, named PSR B0531+21, emits beams of radiation, including X-rays and radio waves, which are observed from Earth. The nebula's intricate filamentary structures and expanding shockwaves are the remnants of the original star's outer layers, now illuminated by the energy released during the explosion. Observations across various wavelengths, from radio to gamma-ray, have provided valuable insights into the dynamics of supernova remnants and the processes occurring in their aftermath.

Comments

Revisions

  • M1 The Crab Nebula, Prodromos
    Original
  • M1 The Crab Nebula, Prodromos
    B
  • Final
    M1 The Crab Nebula, Prodromos
    C

Sky plot

Sky plot

Histogram

M1 The Crab Nebula, Prodromos