最終更新日：2024/08/07
(astronomy, nuclear physics) The explosive ignition of thermonuclear fusion within a carbon-oxygen white dwarf star that occurs when its mass exceeds approximately 1.4 times that of the Sun (due to accretion of material or merger with another star), producing a supernova which completely destroys the star.
正解を見る
carbon detonation
編集履歴（0）
元となった辞書の項目
carbon detonation
noun
(astronomy,
nuclear
physics)
The
explosive
ignition
of
thermonuclear
fusion
within
a
carbon-oxygen
white
dwarf
star
that
occurs
when
its
mass
exceeds
approximately
1.4
times
that
of
the
Sun
(due
to
accretion
of
material
or
merger
with
another
star),
producing
a
supernova
which
completely
destroys
the
star.
意味（1）
(astronomy,
nuclear
physics)
The
explosive
ignition
of
thermonuclear
fusion
within
a
carbon-oxygen
white
dwarf
star
that
occurs
when
its
mass
exceeds
approximately
1.4
times
that
of
the
Sun
(due
to
accretion
of
material
or
merger
with
another
star),
producing
a
supernova
which
completely
destroys
the
star.
