SN 1604

Observation data (Epoch J2000)
SN 1604
A false-color composite (HST/SIRTF) image of the supernova remnant nebula from SN 1604. Credit: HST/NASA/ESA.
Supernova type	Ia ^[1]
Remnant type	Shell
Host galaxy	Milky Way
Constellation	Ophiuchus
Right ascension	17^h 30^m 42^s
Declination	−21° 29′
Galactic coordinates	G4.5+6.8
Discovery date	October 1604
Peak magnitude (V)	−2.25 to −2.5
Distance	20000 light-years, or 6 kpc
Physical characteristics
Progenitor	Unknown
Progenitor type	Unknown
Colour (B-V)	Unknown
Notable features	Last observed supernova in our galaxy. Maintained naked-eye visibility for 18 months.

Supernova 1604, also known as Kepler's Supernova, Kepler's Nova or Kepler's Star, was a supernova which occurred in the Milky Way, in the constellation Ophiuchus. As of 2007^[update], it is the last supernova to have been unquestionably observed in our own galaxy, occurring no farther than 6 kiloparsecs or about 20,000 light-years from Earth. Visible to the naked eye, it was brighter at its peak than any other star in the night sky, and all the planets (other than Venus), with apparent magnitude −2.5.

The supernova was first observed on October 8, 1604 by Johannes Kepler.^[2] ]. It was subsequently named after him due to his book on the subject entitled De Stella nova in pede Serpentarii (On the new star in Ophiuchus's foot).

Johannes Kepler's original drawing depicting the location of the stella nova, marked with an N (8 grid squares down, 4 over from the left).

It was the second supernova to be observed in a generation (after SN 1572 seen by Tycho Brahe in Cassiopeia). No further supernovae have since been observed with certainty in the Milky Way, though many others outside our galaxy have been seen.

The supernova remnant resulting from this supernova is considered to be one of the "prototypical" objects of its kind, and is still an object of much study in astronomy.