Changes

{{Night Sky

{{Night Sky

| image          =

| image          =Keplers supernova.jpg

| designation    =SN 1604<br/>G4.5+6.8

| designation    =SN 1604<br/>G4.5+6.8

| rightascension  =17^h 30^m 41.5^s<ref name=spitzer>[http://www.spitzer.caltech.edu/images/1278-ssc2004-15a1-Composite-View-of-Kepler-s-Supernova-Remnant-SN-1604 Composite View of Kepler's Supernova Remnant - SN 1604] from spitzer.caltech.edu</ref>

| rightascension  =17^h 30^m 41.5^s<ref name=spitzer>[http://www.spitzer.caltech.edu/images/1278-ssc2004-15a1-Composite-View-of-Kepler-s-Supernova-Remnant-SN-1604 Composite View of Kepler's Supernova Remnant - SN 1604] from spitzer.caltech.edu</ref>

Observations in the [[visible light|optical]] regions of the [[electromagnetic spectrum]] have revealed where the shockwave hits high [[density]] regions of gas.<ref name=spitzer/> After the shock wave passes, these denser regions form bright knots and filaments. [[Infrared]] images of the nebula have shown microscopic [[dust]] particles that have been heated by the shockwave and brightest where in the knots and filaments.

Observations in the [[visible light|optical]] regions of the [[electromagnetic spectrum]] have revealed where the shockwave hits high [[density]] regions of gas.<ref name=spitzer/> After the shock wave passes, these denser regions form bright knots and filaments. [[Infrared]] images of the nebula have shown microscopic [[dust]] particles that have been heated by the shockwave and brightest where in the knots and filaments.

==References==

==References==