annular eclipse
a
a
a
nnu
ˈnjʊ
nyoo
lar
lɑ:r
laar
ec
ÉĒk
ik
lipse
lÉĒps
lips
/ɐnjˈʊlɑːɹ ÉĒklˈÉĒps/

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

01

āϕ⧁āĻŖā§āĻĄāϞāĻžāĻ•āĻžāϰ āĻ—ā§āϰāĻšāĻŖ, āϕ⧁āĻŖā§āĻĄāϞāĻžāĻ•āĻžāϰ āϏ⧂āĻ°ā§āϝāĻ—ā§āϰāĻšāĻŖ

a type of solar eclipse where the moon, passing between the earth and the sun, appears smaller than the sun, creating a ring of sunlight around the darkened moon
āωāĻĻāĻžāĻšāϰāĻŖ
An annular eclipse differs from a total solar eclipse because the Moon's apparent size does not completely cover the Sun, leaving a visible ring of sunlight.
āĻāĻ•āϟāĻŋ āĻŦāϞāϝāĻŧāĻžāĻ•āĻžāϰ āĻ—ā§āϰāĻšāĻŖ āϏāĻŽā§āĻĒā§‚āĻ°ā§āĻŖ āϏ⧂āĻ°ā§āϝāĻ—ā§āϰāĻšāĻŖ āĻĨ⧇āϕ⧇ āφāϞāĻžāĻĻāĻž āĻ•āĻžāϰāĻŖ āϚāĻžāρāĻĻ⧇āϰ āφāĻĒāĻžāϤ āφāĻ•āĻžāϰ āϏ⧂āĻ°ā§āϝāϕ⧇ āϏāĻŽā§āĻĒā§‚āĻ°ā§āĻŖāϰ⧂āĻĒ⧇ āφāĻšā§āĻ›āĻžāĻĻāĻŋāϤ āĻ•āϰ⧇ āύāĻž, āϝāĻžāϰ āĻĢāϞ⧇ āϏ⧂āĻ°ā§āϝāĻžāϞ⧋āϕ⧇āϰ āĻāĻ•āϟāĻŋ āĻĻ⧃āĻļā§āϝāĻŽāĻžāύ āĻŦāϞāϝāĻŧ āĻ…āĻŦāĻļāĻŋāĻˇā§āϟ āĻĨāĻžāϕ⧇āĨ¤
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āĻ…ā§āϝāĻžāĻĒ āĻĄāĻžāωāύāϞ⧋āĻĄ āĻ•āϰ⧁āύ