1a. Define: nuclear fusion
the process by which two or more small nuclei fuse to make a bigger nucleus
1b. Define: nuclear fission
the process by which a large nucleus is split into smaller nuclei
1c. Define: critical mass
the amount of isotope necessary to sustain a chain reaction
1d. Define: absolute magnitude
The brightness of a star, corrected for distance, on a scale of -8 to +19. The smaller the number, the brighter the star.
1e. Define: apparent magnitude
The brightness of a star as seen in the night sky. The smaller the number the brighter the star.
1f. Define: light year
the distance light could travel along a straight line in one year
1g. Define: galaxy
a large ensemble of stars, all interacting through the gravitational force and orbiting around a common center
the core, the radiative zone, the convection zone, and the photosphere
the sun gets its power from nuclear fusion that occurs in the core
the photosphere
nuclear fission
nuclear fusion
the mass of the starting materials is larger than the mass of the materials the process makes
a power plant does not have significantly more than the critical mass of the large nucleus that is breaking apart
Nuclear fusion is a better means of producing energy because there are no radioactive byproducts, there is no chance of meltdown, and the starting materials are cheap.
We cannot use nuclear fusion yet because we cannot master the technology to make it economically feasible.
a- Red Giant b-Main Sequence c- Supergiant d-White Dwarf
star (b) is most like our sun
(d), (b), (a) and (c)
(d), (b), (a), and (c)
(a) is the coolest
all three of these are variable star types; thus, their brightness changes radically with time
The big difference between these star types is lifetime. Pulsating stars last a long time, supernovas exist very briefly, and novas are somewhere in between.
most likely formed by a supernova