 |
 |
|
|
|


NADIR
The nadir is the point directly below an observer. |

NAIAD
Naiad is a tiny moon of Neptune. It was discovered using NASA's
Voyager 2 mission in 1989. It orbits 48,230 km from the center
of Neptune and is about 58 km in diameter. |
NANOMETER
A nanometer is unit of measure equal to 10 angstroms, which is
one billionth (1 x 10-9) of a meter. |
NANOROVER
A nanorover (also called small science vehicle or ssv) is a
small rover designed to be sent to explore small celestial
bodies, like asteroids. The book-sized Japanese nanorover MUSES-CN
(MUSES stands for the Mu Space Engineering Spacecraft) will be
sent to explore asteroid 4660 Nereus in Jan. 2002 and arrive on
Nereus on September 9, 2003; it will be the smallest rover ever
to fly on a space mission. It will analyse rock samples, send
color video to Earth, collect rock samples, and will eventually
return to Earth (in 2006). |

NASA
NASA is the National Aeronautics and Space Administration.
|

NEA
NEA stands for Near-Earth Asteroid. NEA's are asteroids whose
orbits bring them within 1.3 AU (121 million miles/195 million
kilometers) of the Sun are called Near-Earth Asteroids (NEA) or
Earth-Approaching asteroids. These asteroids probably came from
the main asteroid belt, but were jolted from the belt by
collisions or interactions with other planets' gravitational
fields. 433 Eros, pictured above, is a NEA. |

NEAP TIDES
Neap tides are especially weak tides. They occur when the
gravitational forces of the Moon and the sun are perpendicular
to one another (with respect to the Earth). Neap tides occur
during quarter moons. |

NEAR PROJECT
NEAR (Near-Earth Asteroid Rendezvous) is a spacecraft designed
to fly by and examine near-earth asteroids. It was launched on
February 17, 1996; its goal was to rendezvous with asteroid 433
Eros (pictured above). In 2001, NASA renamed the spacecraft NEAR
Shoemaker to honor the planetary science pioneer Dr. Eugene M.
Shoemaker, who died in 1997. It orbited Eros from Feb. 14, 2000,
until Feb. 28, 2001, when it landed on Eros. After orbiting the
asteroid Eros (433) for 3 years, NEAR Shoemaker landed on Eros
on Feb 12, 2001 (this was the first spacecraft to land on an
asteroid). After transmitting radio data, the last contact with
NEAR Shoemaker was on Feb. 28, 2001 (it is powered by solar
power). |
NEAT
NEAT (Near-Earth Asteroid Tracking) is a NASA/JPL system that
tracks near-earth asteroids. NEAT uses the 1.2-meter- diameter
(48-inch) Palomar telescope to track asteroids that come close
to the Earth. |

NEBULA
A nebula is a huge, diffuse cloud of gas and dust in
intergalactic space. The gas in nebulae (the plural of nebula)
is mostly hydrogen gas (H2). The plural of nebula is
nebulae or nebulas. |
NEMESIS
Nemesis is a hypothetical companion dark star to our Sun. Once
every 30 million years, this dark star would pass through the
Oort cloud, triggering comets that perhaps cause periodic mass
extinctions on Earth. |
NEO
NEO stands for Near-Earth Object. NEO's are comets and asteroids
that have ventured close to the Earth's orbit. |

NEPTUNE
Neptune is the eighth planet from the sun. It is a cold, gaseous
giant with a hazy atmosphere and is orbited by eight moons and
three narrow, faint rings. |

NEREID
Neptune's outermost moon is Nereid. It is the smaller of
Neptune's 2 larger moons. It has a VERY elliptical orbit, going
as close as 867,000 miles from Neptune and as far as 6 million
miles from it; it may be a captured asteroid. It takes almost
one Earth year for Nereid to orbit Neptune in this extreme
orbit. Nereid's diameter is about 200 miles (320 km). It was
discovered by G. Kuiper in 1949. |
NEREUS
4660 Nereus is a Near-Earth asteroid that is about 0.6 to 1.25
miles (1-2 km) in diameter. It has an orbital period of 1.82 yrs
and a semimajor axis of 1.490 AU. Nereus may be an extinct
comet. MUSES-CN is a Japanese nanorover, a small, book-sized
rover designed to be sent to explore the asteroid Nereus. MUSES
will be launched from Japan in Jan. 2002 and arrive on Nereus on
September 9, 2003; it will be the smallest rover ever to fly on
a space mission. It will analyse rock samples, send color video
to Earth, collect rock samples, and will eventually return to
Earth (in 2006). |
NEUTRINO
A neutrino is an uncharged particle with virtually no mass.
Neutrinos are produced in some nuclear reactions in stars. |

NEUTRON
A neutron is an uncharged atomic nuclear particle. It has a mass
slightly greater than a proton. In beta decay, a neutron decays
into a proton, an electron, and an anti-neutrino. |
NEUTRON STAR
A neutron star is a very small, super-dense star which is
composed mostly of tightly-packed neutrons. This hard-to-see
body has a thin atmosphere of superhot hydrogen plasma and a
crust. It has a diameter of about 5-10 miles (5-16 km) and a
density of roughly 10 15 gm/cm3. Neutron
stars are formed from supernova explosions. |
NEW GENERAL CATALOG
The New General Catalog (NGC) is a list of over 13,000 deep-sky
celestial objects. It was developed in 1888. For example, the
Great Nebula in Orion is NCG 1976 (and M42). |
NEW MOON
The new moon is the phase of the moon when the moon is not
visible from Earth, because the side of the moon that is facing
us is not being lit by the sun. |

NEWTON, ISAAC
Isaac Newton (1642-1727) was an English mathematician and
physicist who invented calculus (simultaneously, but
independently of Leibniz), formulated the laws of gravitation,
investigated the nature of light (he discovered that sunlight is
made of light of different colors), and the laws of motion:
1. An object in uniform motion tends to remain in that state
of motion unless an external force is applied to it (the Law of
Inertia). 2. A force causes a change in the velocity
(acceleration) of an object (F=ma). 3. For every
action there is an equal and opposite reaction. Newton also
improved the design of the refracting telescope (using an
objective mirror, instead of a lens), and it is now called a
Newtonian telescope. |

NGC
The NGC (New General Catalog) is a list of over 13,000 deep-sky
celestial objects. It was developed in 1888. For example, the
Great Nebula in Orion is NCG 1976 (and M42). NGC4414 (pictured
above) is a spiral galaxy 60 million light-years away. |
NOCTILUCENT CLOUD
Noctilucent clouds (abbreviated "NLC") are very high-altitude
clouds that are visible at night in June and July from the
latitudes 50 to 65 degrees. These clouds are at roughly 82-85 km
altitude, a dry part of the atmosphere. Noctilucent means "night
shine." Noctilucent clouds are probably made of small ice-coated
particles. Not very much is currently known about these clouds.
Noctilucent clouds were named in 1884. |

NORTHERN LIGHTS
Northern lights is another name for auroras that appear in the
Northern Hemisphere. Auroras are beautiful undulating sheets of
light in the near-polar sky. They are caused by gases that
become excited after being hit by solar particles. Most auroras
are 100 to 250 km above the ground. |

NORTH STAR
The north star is a star that is located almost due north and is
useful for navigation. Polaris is currently the pole star of the
Northern Hemisphere. |

NOVA
A nova is a white dwarf star that suddenly increases in
brightness by several magnitudes. It fades very slowly. |
NUCLEAR BULGE
The nuclear bulge is the central, spherical part of a spiral
galaxy. It is surrounded by a disk-shaped mass of stars with
spiral arms. |
NUCLEAR FISSION
Nuclear fission is a reaction in which an atom's nucleus is
broken apart, releasing a tremendous amount of energy. Nuclear
fission is used in many power plants on Earth (and is used in
atomic weapons). Nuclear fission is not an important reaction in
the Sun (for nuclear fission, the nuclear reaction that occurs
in the Sun, click here). |

NUCLEAR FUSION
Nuclear fusion is an atomic reaction in which many nuclei (the
centers of atoms) combine together to make a larger one (which
is a different element). The result of this process is the
release of a lot of energy (the resultant nucleus is smaller in
mass than the sum of the ones that made it; the difference in
mass is converted into energy by the equation E=mc2).
Suns are powered by nuclear fusion, mostly converting hydrogen
into helium. In this process, 4 hydrogen nuclei combine to form
a single helium nucleus; about 0.3% of the original mass is
converted into energy. |
NUCLEOSYNTHESIS
Nucleosynthesis is the production of new elements via nuclear
reactions. Nucleosynthesis takes place in stars. It also took
place soon after the Big Bang. |

NUCLEUS
The nucleus of an atom is its center, which contain most of the
atom's mass; in the nucleus is everything but the orbiting
electrons. |

NUCLEUS
The nucleus is the frozen center of a comet's head. The nucleus
contains most of the comet's mass. |
|
 |
|