This is a list of observed supernova remnants (SNRs) in the Milky Way, as well as galaxies nearby enough to resolve individual nebulae, such as the Large and Small Magellanic Clouds and the Andromeda Galaxy.
Supernova remnants typically only survive for a few tens of thousands of years, making all known SNRs fairly young compared to many other astronomical objects.
Image | Name | Right ascension | Declination | First visible from Earth | Peak magnitude | Distance (ly) | Type | Remnant | |
---|---|---|---|---|---|---|---|---|---|
Sh2-264 or Lambda Orionis Ring | ~1 million years ago | ? | 1,100 | ? | ? | ||||
Sagittarius A East | 100,000−35,000 years ago | ? | 26,000 | tidal disruption | ? | ||||
Monogem Ring (SNR G201.1+08.3) | ~86,000 years ago | ? | 900 | ? | neutron star PSR B0656+14 | ||||
Simeis 147 or Spaghetti Nebula | ~40,000 years ago | 6.5 | 3,000 | ? | neutron star PSR J0538+2817 | ||||
scope=“row” | IC 443 also known as jellyfish nebulae | ~30,000 years ago | ? | 3,000 | neutron star CXOU J061705.3+222127 | ||||
SNR G132.6+01.5 | 33,000–27,000 years ago | ? | 7,200 | ? | ? | ||||
W50 or Manatee Nebula | ~20,000 years ago | ? | 18,000 | ? | black hole/neutron star SS 433 | ||||
W44 | 20,000–16,000 years ago | ? | 10,400 | ? | neutron star PSR B1853+01 | ||||
SNR G359.0-0.9 | 18,000 years ago | ? | 11,000 | ? | ? | ||||
Vela SNR | 10,300−9,000 BCE | 12 | neutron star Vela Pulsar | ||||||
SNR G359.1-0.5 | ca. 8,000 BCE[1] | ? | 10,500 | ? | ? | ||||
CTB 1 or Abell 85 | 9,000–5,500 BCE | ? | 10,100 | ? | neutron star PSR J0002+6216 | ||||
Kesteven 79 | 8600–7000 BCE | ? | 23,000 | ? | neutron star PSR J1852+0040 | ||||
| Cygnus Loop, including Veil Nebula | 6,000−3,000 BCE | 7 | 1,470 | ? | possible neutron star 2XMM J204920.2+290106 | |||
scope=“row” | 3C 58 | 3500−1500 BCE | ? | 8,000 | ? | pulsar 3C 58 | |||
LMC N49 | ~3,000 BCE | ? | 160,000 | ? | neutron star PSR B0525-66 | ||||
G299.2-2.9[2] | ~2,500 BCE | ? | 16,000 | none | |||||
Puppis A | ~1,700 BCE | ? | 7,000 | ? | neutron star RX J0822−4300 | ||||
G332.4+00.1 | ~1,000 BCE | ? | 16,800 | ? | neutron star PSR J1614-5048 | ||||
G54.1+0.3[3] | ~900 BCE | ? | 22,000 | ? | neutron star PSR J1930+1852 | ||||
G292.0+01.8 | ~800–400 BCE | ? | 17,600 | ? | neutron star PSR J1124-5916 | ||||
Kesteven 75 | 1st millennium BCE | ? | 18,900 | ? | neutron star PSR J1846-0258 | ||||
G306.3-0.9[4] | ~400 BCE | ? | 26,000 | Ia | none | ||||
RCW 103 | 1st century | ? | 10,000 | neutron star 1E 161348-5055 | |||||
SN 185 | ? | 8,200 | none | ||||||
CTB 37B (possibly SN 393) | ~500 CE (April 393?) | ? | 43,000 | ? | neutron star CXOU J171405.7-381031 | ||||
E0102 | 1st millennium | ? | 190,000 | ? | neutron star | ||||
SNR 0540-69.3 | 350–1250 CE | ? | 160,000 | ? | neutron star PSR J0540−6919 | ||||
W49B | About 1000 CE | ? | 26,000 | unidentified black hole | |||||
SN 1006 | -7.5 | 7,200 | Ia[5] | none | |||||
G350.1-0.3 | 1000–1100 | ? | 15,000 | ? | neutron star XMMU J172054.5-372652 | ||||
SN 1054 or M1 or Crab Nebula | -6 | 6,300 | neutron star Crab Pulsar | ||||||
RX J0852.0-4622 or Vela Junior | September 13, 1271[6] | ? | 700 | ? | neutron star CXOU J085201.4–461753 | ||||
SGR 1806-20 | 1050–1650 | ? | 42,000 | ? | neutron star SGR 1806-20 | ||||
SN 1572 or Tycho's Nova | -4 | 7,500 | none | ||||||
SN 1604 or Kepler's Nova | -2.5 | 20,000 | none | ||||||
Cassiopeia A | circa 1667 | 6 | 10,000 | IIb[7] | neutron star CXOU J232327.8+584842 | ||||
SN 1885A or S Andromedae | 6 | 2,500,000 | I pec | none | |||||
G1.9+0.3 | circa 1898 | ? | 25,000 | none | |||||
SN 1987A | 3 | 168,000 | neutron star |