by NGC3314 » Sun Feb 24, 2019 8:18 pm
JohnD wrote: ↑Sun Feb 24, 2019 3:16 pm
The APOD blurb doesn't say why there are two expanding reflection rings. Did Supernova 1987A explode twice?
For each value of the time delay (time since we served the direct light of the explosion), there is a locus of possible light echos which is an ellipse with the observer and the supernova at the foci. We will, in princjple, see echoes from anywhere on this ellipse where there is enough scattering material (in practice, interstellar dust forward-scatters light very strongly and backscatters very weakly, so material near the SN is easier to see). Multiple rings correspond to multiple density enhancements along the line of sight. For SN1987A, they imply fairly narrow sheets of dust in the Large Magellanic Cloud one of which is tilted to the line of sight as shown by its ring being off-center to the SN direction.
Because they do not correspond to moving material objects, it is possible for the projected locations of light echoes to move faster than c - in fact the combination of apparent velocity and time delay can give the distance to the scattering material. Using this property, light echoes have been identified from Cassiopeia A and Tycho's supernova, and the reflected spectra provided classifications of the explosions.
[quote=JohnD post_id=290109 time=1551021389 user_id=100329]
The APOD blurb doesn't say why there are two expanding reflection rings. Did Supernova 1987A explode twice?
[/quote]
For each value of the time delay (time since we served the direct light of the explosion), there is a locus of possible light echos which is an ellipse with the observer and the supernova at the foci. We will, in princjple, see echoes from anywhere on this ellipse where there is enough scattering material (in practice, interstellar dust forward-scatters light very strongly and backscatters very weakly, so material near the SN is easier to see). Multiple rings correspond to multiple density enhancements along the line of sight. For SN1987A, they imply fairly narrow sheets of dust in the Large Magellanic Cloud one of which is tilted to the line of sight as shown by its ring being off-center to the SN direction.
Because they do not correspond to moving material objects, it is possible for the projected locations of light echoes to move faster than c - in fact the combination of apparent velocity and time delay can give the distance to the scattering material. Using this property, light echoes have been identified from Cassiopeia A and Tycho's supernova, and the reflected spectra provided classifications of the explosions.