Oceanography before the earth chapter 1 Flashcards
Big Bang
about 13.7 billion years ago, a plethora of stars and galaxies emerged that hosted planets and possibly the ingredients necessary for life itself.
Nebula
gas or dust that may either be dark or may glow. Most of the gas we see in the universe is hydrogen gas. When illuminated by nearby stars a nebula will glow.
Galaxy
a collection of stars and nebula that clustered around a center of mass of very dense material. Many believe that the center of most galaxies might consist of a supermassive black hole (the collapsed remnant of a massive star from which no light can escape due to the strength of its gravitational field).
Stars
massive bodies of incandescent gases like hydrogen and helium that form from the condensation of a nebula
Thermonuclear Fusion
a nuclear reaction that produces so much energy that it pushes stellar material outward
Gravity
a force due to the presence of a mass that pulls the mass of the star inward
Plasma
is the fourth state of matter and can be described as a hot gas-like mass of ions that can be influenced by electromagnetic fields. It is the most common state of matter in the universe.
Proto- Star
This phase of star formation lasts about 1 million years for a star the size of our Sun.
Main-sequence star
Once gravity and fusion are balanced and the core temperature reaches 10 million degrees, the star is considered a stable main-sequence star
Annealing
As the density of the larger masses increased, they melted and fused in a process called annealing.
Red giant
the size of the star expands into the red giant
White dwarf
The star will collapse into a very massive object (a white dwarf (defined below), in the case of our Sun)
Planetary nebula
The collapse by gravity results in a blast shedding outer gases called a planetary nebula
Supernova
The collapse by gravity results in a supernova blast
Dark matter
Our universe contains a remarkable amount of material and much of it is not even visible to the naked eye. There is still a large amount of this matter called dark matter that has yet to be observed and explained.