nebular hypothesis
ne
ˈnɛ
ne
bu
bjƊ
byoo
lar
lər
lēr
hy
haÉĒ
hai
po
pɑ:
paa
the
θə
thē
sis
ˌsÉĒs
sis
/nˈɛbjƊlə haÉĒpˈɒθəsˌÉĒs/

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

01

āύ⧀āĻšāĻžāϰāĻŋāĻ•āĻž āĻ…āύ⧁āĻŽāĻžāύ, āύ⧀āĻšāĻžāϰāĻŋāĻ•āĻž āϤāĻ¤ā§āĻ¤ā§āĻŦ

(cosmology) a theory proposing that the solar system formed from a rotating nebula of gas and dust about 4.6 billion years ago
āωāĻĻāĻžāĻšāϰāĻŖ
According to the nebular hypothesis, the planets formed from the leftover material.
āύ⧇āĻŦ⧁āϞāĻžāϰ āĻšāĻžāχāĻĒā§‹āĻĨāĻŋāϏāĻŋāϏ āĻ…āύ⧁āϝāĻžāϝāĻŧā§€, āĻ—ā§āϰāĻšāϗ⧁āϞāĻŋ āĻ…āĻŦāĻļāĻŋāĻˇā§āϟ āωāĻĒāĻžāĻĻāĻžāύ āĻĨ⧇āϕ⧇ āĻ—āĻ āĻŋāϤ āĻšāϝāĻŧ⧇āĻ›āĻŋāϞāĨ¤
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āύāĻŋāĻ•āϟāĻŦāĻ°ā§āϤ⧀ āĻļāĻŦā§āĻĻ
LanGeek
āĻ…ā§āϝāĻžāĻĒ āĻĄāĻžāωāύāϞ⧋āĻĄ āĻ•āϰ⧁āύ