The Full Wiki



More info on SN 1604

SN 1604: Wikis

  

Note: Many of our articles have direct quotes from sources you can cite, within the Wikipedia article! This article doesn't yet, but we're working on it! See more info or our list of citable articles.

Encyclopedia

Updated live from Wikipedia, last check: June 04, 2012 10:30 UTC (43 seconds ago)

From Wikipedia, the free encyclopedia

SN 1604
Keplers supernova.jpg
A false-color composite (HST/SIRTF) image of the supernova remnant nebula from SN 1604.
Credit: HST/NASA/ESA.
Observation data (Epoch J2000)
Supernova type Ia [1]
Remnant type Shell
Host galaxy Milky Way
Constellation Ophiuchus
Right ascension 17h 30m 42s
Declination −21° 29′
Galactic coordinates G4.5+6.8
Discovery date October 1604
Peak magnitude (V) −2.25 to −2.5
Distance 20,000 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 2009, 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 in northern Italy on October 9, 1604. Johannes Kepler began observing it on October 17.[2] It was subsequently named after him because of 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.

See also

References

  1. ^ "Chandra X-Ray Observatory". Kepler's Supernova Remnant: A Star's Death Comes to Life. http://chandra.harvard.edu/photo/2007/kepler/index.html. Retrieved 2006-01-16.  
  2. ^ Bill Blair's Kepler's Supernova Remnant Page Accessed October 7, 2009

External links

Coordinates: Sky map 17h 30m 38.5s, −21° 28′ 48″








Got something to say? Make a comment.
Your name
Your email address
Message
Please enter the solution to case below
12+12=