|
+ big_bang
|
n
|
1
|
[ cosmogeny ]
|
eng-30-07408796-n
|
(cosmology) the cosmic explosion that is hypothesized to have marked the origin of the universe
|
|
+ big_bang_theory
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05887911-n
|
(cosmology) the theory that the universe originated sometime between 10 billion and 20 billion years ago from the cataclysmic explosion of a small volume of matter at extremely high density and temperature
|
|
+ big-bang_theory
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05887911-n
|
(cosmology) the theory that the universe originated sometime between 10 billion and 20 billion years ago from the cataclysmic explosion of a small volume of matter at extremely high density and temperature
|
|
+ CBR
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ closed_universe
|
n
|
1
|
[ cosmogeny ]
|
eng-30-09247071-n
|
(cosmology) a universe that is spatially closed and in which there is sufficient matter to halt the expansion that began with the big bang; the visible matter is only 10 percent of the matter required for closure but there may be large amounts of dark matter
|
|
+ CMB
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ CMBR
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ continuous_creation_theory
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05888572-n
|
(cosmology) the theory that the universe maintains a constant average density with matter created to fill the void left by galaxies that are receding from each other
|
|
+ cosmic_background_radiation
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ cosmic_microwave_background
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ cosmic_microwave_background_radiation
|
n
|
1
|
[ cosmogeny ]
|
eng-30-11441077-n
|
(cosmology) the cooled remnant of the hot big bang that fills the entire universe and can be observed today with an average temperature of about 2.725 kelvin
|
|
+ cosmic_string
|
n
|
1
|
[ cosmogeny ]
|
eng-30-09449282-n
|
(cosmology) a hypothetical one-dimensional subatomic particle having a concentration of energy and the dynamic properties of a flexible loop
|
|
+ cosmogenic
|
a
|
1
|
[ cosmogeny ]
|
eng-30-02703438-a
|
pertaining to the branch of astronomy dealing with the origin and history and structure and dynamics of the universe
|
|
+ cosmogonic
|
a
|
1
|
[ cosmogeny ]
|
eng-30-02703438-a
|
pertaining to the branch of astronomy dealing with the origin and history and structure and dynamics of the universe
|
|
+ cosmogonical
|
a
|
1
|
[ cosmogeny ]
|
eng-30-02703438-a
|
pertaining to the branch of astronomy dealing with the origin and history and structure and dynamics of the universe
|
|
+ cosmologic
|
a
|
1
|
[ cosmogeny ]
|
eng-30-02703438-a
|
pertaining to the branch of astronomy dealing with the origin and history and structure and dynamics of the universe
|
|
+ cosmological
|
a
|
1
|
[ cosmogeny ]
|
eng-30-02703438-a
|
pertaining to the branch of astronomy dealing with the origin and history and structure and dynamics of the universe
|
|
+ Hubble_constant
|
n
|
1
|
[ cosmogeny ]
|
eng-30-13590598-n
|
(cosmology) the ratio of the speed of recession of a galaxy (due to the expansion of the universe) to its distance from the observer; the Hubble constant is not actually a constant, but is regarded as measuring the expansion rate today
|
|
+ Hubble_parameter
|
n
|
1
|
[ cosmogeny ]
|
eng-30-13590598-n
|
(cosmology) the ratio of the speed of recession of a galaxy (due to the expansion of the universe) to its distance from the observer; the Hubble constant is not actually a constant, but is regarded as measuring the expansion rate today
|
|
+ Hubble's_constant
|
n
|
1
|
[ cosmogeny ]
|
eng-30-13590598-n
|
(cosmology) the ratio of the speed of recession of a galaxy (due to the expansion of the universe) to its distance from the observer; the Hubble constant is not actually a constant, but is regarded as measuring the expansion rate today
|
|
+ Hubble's_parameter
|
n
|
1
|
[ cosmogeny ]
|
eng-30-13590598-n
|
(cosmology) the ratio of the speed of recession of a galaxy (due to the expansion of the universe) to its distance from the observer; the Hubble constant is not actually a constant, but is regarded as measuring the expansion rate today
|
|
+ inflation
|
n
|
2
|
[ cosmogeny ]
|
eng-30-07409255-n
|
(cosmology) a brief exponential expansion of the universe (faster than the speed of light) postulated to have occurred shortly after the big bang
|
|
+ nebular_hypothesis
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05888215-n
|
(cosmology) the theory that the solar system evolved from a hot gaseous nebula
|
|
+ planetesimal_hypothesis
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05888377-n
|
(cosmology) the theory that the solar system was formed by the gravitational accumulation of planetesimals
|
|
+ steady_state_theory
|
n
|
1
|
[ cosmogeny ]
|
eng-30-05888572-n
|
(cosmology) the theory that the universe maintains a constant average density with matter created to fill the void left by galaxies that are receding from each other
|
|
+ string
|
n
|
8
|
[ cosmogeny ]
|
eng-30-09449282-n
|
(cosmology) a hypothetical one-dimensional subatomic particle having a concentration of energy and the dynamic properties of a flexible loop
|
