type II supernova Comparison Table

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type II supernova comparison table

Subject has energy release has spectral type is part of has extent has age has surface temperature has velocity is an instance of has frequency has surface density has optical brightness variation has star surface temperature has V magnitude has parallax has light curve has observational problem has position on celestial sphere has location has angular momentum has distance has radiation at surface has acronym has B magnitude has temperature has recovery time has spectra has proper motion has amplitude has energy source has energy production has catalog has outburst start time has absolute magnitude has U magnitude has volume has momentum has peak brightness has apparent magnitude has material has mass has ejecta velocity has image has name designated with has observable variation time scale has emission line has use has synonym

SN 1987A 10⁴⁹ to 10⁵¹ ergs Large Magellanic Cloud greater than 1000 Kelvin determined from proper motion and radial velocity type II supernova 0.01 to 0.05 per year (in our Galaxy) which depends on luminosity class 0.2 magnitudes or greater from the point of view of Earth's orbit some difficulty in distinguishing between various kinds from the point of view of Earth young, massive stars near the edge of spiral arms 167000 light years which is diffused out from the hotter core CV hydrogen lines gravitational contraction and or fusion which takes place primarily within the core star catalog M_v = - 12 to - 13.5 10⁸ solar luminosity units hydrogen, helium higher than type II supernova 5000 km s^-1
R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
V 335, V 336, etc., when the double letter designations are exhausted
within a period of decades supernova peak brightness distance determination explosive variable

Next supernova: type III supernova Up: supernova Previous supernova: type I supernova

Subject	has energy release	has spectral type	is part of	has extent	has age	has surface temperature	has velocity	is an instance of	has frequency	has surface density	has optical brightness variation	has star surface temperature	has V magnitude	has parallax	has light curve	has observational problem	has position on celestial sphere	has location	has angular momentum	has distance	has radiation at surface	has acronym	has B magnitude	has temperature	has recovery time	has spectra	has proper motion	has amplitude	has energy source	has energy production	has catalog	has outburst start time	has absolute magnitude	has U magnitude	has volume	has momentum	has peak brightness	has apparent magnitude	has material	has mass	has ejecta velocity	has image	has name designated with	has observable variation time scale	has emission line	has use	has synonym
SN 1987A	10⁴⁹ to 10⁵¹ ergs		Large Magellanic Cloud			greater than 1000 Kelvin	determined from proper motion and radial velocity	type II supernova	0.01 to 0.05 per year (in our Galaxy)	which depends on luminosity class	0.2 magnitudes or greater			from the point of view of Earth's orbit		some difficulty in distinguishing between various kinds	from the point of view of Earth	young, massive stars near the edge of spiral arms		167000 light years	which is diffused out from the hotter core	CV				hydrogen lines			gravitational contraction and or fusion	which takes place primarily within the core	star catalog		M_v = - 12 to - 13.5				10⁸ solar luminosity units		hydrogen, helium	higher than type II supernova	5000 km s^-1		R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted V 335, V 336, etc., when the double letter designations are exhausted	within a period of decades		supernova peak brightness distance determination	explosive variable