Download Chapter 4 Vocabulary

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Big Bang wikipedia , lookup

Corona discharge wikipedia , lookup

Solar wind wikipedia , lookup

P-nuclei wikipedia , lookup

Astrophysical X-ray source wikipedia , lookup

First observation of gravitational waves wikipedia , lookup

Heliosphere wikipedia , lookup

Corona wikipedia , lookup

Outer space wikipedia , lookup

Cygnus X-1 wikipedia , lookup

Hayashi track wikipedia , lookup

Gravitational lens wikipedia , lookup

Planetary nebula wikipedia , lookup

Nucleosynthesis wikipedia , lookup

Cosmic distance ladder wikipedia , lookup

Standard solar model wikipedia , lookup

Main sequence wikipedia , lookup

Chronology of the universe wikipedia , lookup

H II region wikipedia , lookup

Stellar evolution wikipedia , lookup

Astronomical spectroscopy wikipedia , lookup

Star formation wikipedia , lookup

Transcript
Chapter 4
Vocabulary
Stars, Galaxies, and the
Universe
the moment in time when the
universe started to expand out of
an extremely hot, dense state
big bang
the process in which particles of an
element collide and combine to form
a heavier element
fusion
a cloud of gas and dust in space,
where stars can form
nebula
the apparent shift in position of an
object when viewed from different
locations
parallax
the transfer of energy from place to
place by the motion of heated liquid
or gas
convection
a change in the observed
frequency of a wave, occurring
when the source of the wave or the
observer is moving
Doppler effect
the stage in the life cycle of stars
during which stars produce energy
by fusing hydrogen and helium
main sequence
the distance light travels I one year,
which is about 9.5 trillion kilometers
of 6 trillion miles
light-year
the outer layer of the Sun’s
atmosphere
corona
the very bright center of a distant
galaxy
quasar
a dense core that may be left behind
after a higher-mass star explodes into a
supernova
neutron star
a stream of electrically charged
particles that flows out in all
directions from the Sun’s corona
solar wind
a darker, cooler spot on the
photosphere
sun spot
the final stage of an extremely massive
star, which is invisible because its
gravity prevents any form of radiation
from escaping
black hole