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Glossary links (select a letter for definitions of astronomy terms
beginning with that letter):
A - B - C - D - E - F - G - H - I - J - K - L - M - N - O - P - Q - R - S - T - U - V - W - X - Y - Z
- nanometer
- a very tiny distance equal to one-billionth of
a meter (0.000000001 meter).
- natural selection
- the primary mechanism of evolution by which, over time, heritable traits that enhance survival and successful reproduction will become progressively more common in succeeding generations in any local environment. It is a NON-random process that produces adaptations.
- neap tide
- tide that has a small change between low and high
tide. It occurs at first and third quarter phase, when the Moon's tidal effect is
perpendicular with the Sun's tidal effect.
- neutrino
- a sub-atomic particle with very small mass that is produced in
nuclear fusion reactions and rarely interacts with ordinary matter.
Neutrinos travel at the nearly the speed of light and provide current
information about the number of nuclear fusion reactions occurring in a
star's core (in the case of the Sun, the information is only about 8.3 minutes
old).
- neutron
- subatomic particle with zero charge (neutral charge) that is
found in the nucleus of an atom. It is slightly more massive than the
positively-charged proton.
- neutron degeneracy pressure
- pressure exerted by a degenerate
gas made of neutrons. It is what prevents further
collapse of a neutron star.
- neutron star
- the collapsed core for an intermediate to high-mass
star. The core is more than 1.4 solar masses but less than 3 solar masses
and is about the diameter of a
city. The pressure from degenerate neutrons prevents further collapse.
- newton
- unit of force in the metric system. It is used
to specify the amount of weight.
- Newton's 1st law
- (of motion): a body at rest remains at rest, and one
moving in a straight line maintains a constant speed and same direction unless it is
deflected by a force.
- Newton's 2nd law
- (of motion): the amount of force needed to cause an
acceleration depends on an object's mass, such that the force applied = the mass of an
object × its acceleration.
- Newton's 3rd law
- (of motion): for every action force ON an object, there
is an equal but opposite force BY the object.
- north celestial pole
- (NCP): projection of the Earth's north pole onto
the sky. The NCP altitude = the observer's
northern latitude.
- nova
- an object that greatly increases in brightness
rapidly, so it appears as a ``new star''. It is caused by the buildup
on a white dwarf's surface of hydrogen gas from a companion star to
the point where the hydrogen fuses explosively into helium. The
super-rapid fusion does not blow up the white dwarf, so the process
can repeat itself (contrast with a Type I supernova).
- nuclear fusion
- the process used by stars to generate energy:
less-massive nuclei are fused together under extremely high
temperatures and densities to form more-massive nuclei plus some energy.
The energy comes from the transformation of some of the mass into energy.
- nucleus
- (comet): the ``dirty iceberg'' about the size of a city from which
all of the stuff in a comet comes from. Irregularly-shaped it is made of dust and
frozen gases.
Glossary links (select a letter for definitions of astronomy terms
beginning with that letter):
A - B - C - D - E - F - G - H - I - J - K - L - M - N - O - P - Q - R - S - T - U - V - W - X - Y - Z
last updated: 27 May 2001
Is this page a copy of Strobel's
Astronomy Notes?
Author of original content:
Nick Strobel