supernova
su
su:
soo
per
pər
pēr
no
noƊ
now
va
və
vē
/sˈuːpənˈə‌ʊvɐ/
SN

āχāĻ‚āϰ⧇āϜāĻŋāϤ⧇ "supernova"āĻāϰ āϏāĻ‚āĻœā§āĻžāĻž āĻ“ āĻ…āĻ°ā§āĻĨ

01

āϏ⧁āĻĒāĻžāϰāύ⧋āĻ­āĻž

an exploding star that as a result is emitting a very large amount of light, more than the sun
āωāĻĻāĻžāĻšāϰāĻŖ
The remnants of a supernova can form nebulae and enrich the interstellar medium with heavy elements.
āĻāĻ•āϟāĻŋ āϏ⧁āĻĒāĻžāϰāύ⧋āĻ­āĻž āĻāϰ āĻ…āĻŦāĻļāĻŋāĻˇā§āϟāĻžāĻ‚āĻļ āύ⧀āĻšāĻžāϰāĻŋāĻ•āĻž āĻ—āĻ āύ āĻ•āϰāϤ⧇ āĻĒāĻžāϰ⧇ āĻāĻŦāĻ‚ āĻ­āĻžāϰ⧀ āωāĻĒāĻžāĻĻāĻžāύ āĻĻāĻŋāϝāĻŧ⧇ āφāĻ¨ā§āϤāσāύāĻžāĻ•ā§āώāĻ¤ā§āϰāĻŋāĻ• āĻŽāĻžāĻ§ā§āϝāĻŽāϕ⧇ āϏāĻŽā§ƒāĻĻā§āϧ āĻ•āϰāϤ⧇ āĻĒāĻžāϰ⧇āĨ¤
LanGeek
āĻ…ā§āϝāĻžāĻĒ āĻĄāĻžāωāύāϞ⧋āĻĄ āĻ•āϰ⧁āύ