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ABERRATION OF LIGHT
The
aberration of light is a phenomenon in which light appears to
be slanted (the angle at which the light appears to be coming is
different than the angle at which it's actually coming) if the
observer is in motion. (An analogous situation is watching rain
fall from a moving train - although a raindrop is falling straight
to the ground, it will appear to fall at a slant, and the slant
increases as the train's speed increases.) The aberration of light
is due to the fact that light travels at a finite speed (as do the
raindrops). The aberration of light was discovered and
demonstrated by James Bradley (an English amateur astronomer) in
1725. The discovery of the aberration of light was one of the
first proofs that the speed of light was finite; it also provided
an early estimate of the speed of light (Bradley calculated that
the time it took for light to travel from the Sun to the Earth was
8 minutes and 12 seconds). |
ABLATION
Ablation is a cooling process in which heat is carried away from
an object (like a falling
meteorite) as the flow of air blows away the hot, melted or
vaporized outer layers of the object. Some spacecraft use ablative
heat shields; their outer surface is coated with heat-dissipating
material (like a phenolic epoxy resin, a reinforced plastic) that
burns rapidly, and then falls away during re-entry.
|
| Star |
Absolute Magnitude |
Apparent Magnitude |
Distance from Earth
(light-years) |
|
The Sun |
+4.8 |
-26.72 |
0.000016 |
| Sirius |
+1.4 |
-1.46 |
8.6 |
| Canopus |
-2.5 |
-0.72 |
74 |
| Rigel Kentaurus |
+4.4 |
-0.27 |
4.3 |
| Arcturus |
+0.2 |
-0.04 |
34 |
| Vega |
+0.6 |
0.03 |
25 |
| Capella |
+0.4 |
+0.08 |
41 |
| Rigel |
-8.1 |
+0.12 |
900 |
| Betelgeuse |
-7.2 |
+0.7 |
1,500 |
ABSOLUTE MAGNITUDE
Absolute magnitude is a measure of the inherent
brightness of a celestial object. This scale is defined as the
apparent magnitude a star would have if it were seen from a
standard distance of 32.6 light-years (10 parsecs). The lower the
number, the brighter the object. Negative numbers indicate extreme
brightness.
|

ABSOLUTE ZERO
At absolute zero, a hypothetical temperature, all molecular
movement stops. All actual temperatures are above absolute zero.
Absolute zero would occur at -273.16°C, -459.69°F, or 0 K. |

ABSORPTION LINES
Absorption Lines are dark lines superimposed over a bright
continuous absorption spectrum. Each dark line is formed as a
cooler gas absorbs photons emitted by a particular element from a
hotter source. |

ABSORPTION SPECTRUM
An absorption spectrum (also called a dark-line spectrum) consists
of dark absorption lines superimposed on a bright
continuous spectrum. An absorption spectrum is created when
light from an
incandescent source passes through a cooler gas that absorbs
photons. Each different element and molecule absorbs light at a
unique set of frequencies. Astronomers can determine the
composition of gases in stars by looking for their characteristic
frequencies (this is called
spectroscopy). |
ACCELERATION
Acceleration is the rate of change of velocity. When an object is
moving at a constant velocity (or if it is standing still) it has
zero acceleration. An object whose velocity is increasing has a
positive acceleration. |

ACCRETION DISK
An accretion disk is a flat disk of gas and dust in space that
surrounds a newborn star, black hole, or other enormous object
that is growing by attracting matter to it with its gravitational
field. |

ACHONDRITIC METEORITE
An achondritic meteorite is a stony
meteorite, coarsely crystallized, with large bits of various
minerals visible to the naked eye. |

ACID RAIN
Acid rain is polluted and harmful to the environment. Acid rain
may have been a component of the
K-T extinction. |

ACRUX
Acrux (also known and alpha Crux) is a first magnitude star in the
Southern Hemisphere
constellation Crux (the
Southern Cross). |
ACTIVE GALACTIC NUCLEI
Active galactic nuclei (AGN) are galaxies that have a massive
black hole at the galactic center (nucleus). These galaxies
produce huge amounts of energy (at all wavelengths of the
electromagnetic spectrum). They produce more energy than the just
the total energy emitted from all of the stars in the nebula. AGN
may be related to
starburst galaxies. |
ACTIVE GALAXY
An active galaxy is a galaxy that produces huge amounts of energy;
they produce more energy than the total energy emitted from all of
the stars in the nebula. There may be at least three types of
active galaxies, including Seyfert galaxies,
quasars, and blazars (although these three may be the same
type of galaxy viewed from different distances and perspectives). |
ADAMS, JOHN C.
John Couch Adams (1819-1892) was an English
astronomer and mathematician who, at 24 years old, predicted
the existence of the planet
Neptune (Le
Verrier also predicted its existence, independently). |
ADAPTIVE OPTICS
Adaptive optics (AO) is a process in which distortions (like those
from the Earth's atmosphere) are removed from a telescope's image
in real time. First, a wavefront sensor uses a reference star to
measure the distortions that are occurring. The distortions are
then removed with a phase corrector. AO was recently installed on
the
Keck II telescope in Hawaii, |

ADRASTEA
Adrastea is one of
Jupiter's 16 moons, and the second-closest to Jupiter.
Adrastea is 12 miles (20 km) in diameter and orbits 80,000 miles
(129,000 km) from Jupiter, within its main ring. Adrastea and the
first moon, Metis, are probably the source of the dust in this
ring. Adrastea has a mass of 1.91 x 1016kg.
It orbits Jupiter in 0.29826 (Earth) days; this is faster than
Jupiter rotates on its axis. Adrastea was discovered by D. Jewitt
and E. Danielson (Voyager 2) in 1979. |
AEROLITE
An aerolite is a
meteorite that is consists mostly of stony matter. |
AFTERGLOW
1. An afterglow is a wide arc of glowing light that can sometimes
be seen high in the western sky at twilight; it is caused by fine
particles of dust scattering light in the upper atmosphere. 2. An
afterglow (also called postluminescence) is lingering radiation
that remains after an event like the big bang (whose afterglow is
the the cosmic microwave background radiation) or a gamma ray
burst (which has an x-ray afterglow). |
AIMPOINT
An aimpoint is a point in the plane of a planet's orbit that a
spacecraft aims for (either for a fly by of that planet or to
enter that planet's orbit). |
AIRY, GEORGE
Sir George Bidell Airy (1801-1892) was the director of
Greenwich Observatory/Astronomer Royal of England from 1835 to
1881. Airy installed a transit (a precise surveying device) at
Greenwich, England, which was used to define the zero degree
meridian of the Earth (zero-degrees longitude). A crater on Mars
about 5 degrees south of the equator and on what is defined as
Mars' prime meridian (zero-degrees longitude) is call Airy. A
small crater within this crater (which is called Airy-0) is where
the meridian line (zero-degrees longitude) crosses. A crater on
the moon is also named for him (latitude 18.1 degrees, longitude
354.3 degrees, diameter 36 km). Airy is supposed to have stated
incorrectly that Charles Babbage's new "analytical engine" (the
predecessor of the computer) was "worthless," effectively ending
Babbage's government funding. |
| Planet |
Albedo |
|
Mercury |
0.12 |
|
|
Venus |
0.59 |
|
|
Earth |
0.39 |
|
|
Mars |
0.15 |
|
|
Jupiter |
0.44 |
|
|
Saturn |
0.46 |
|
|
Uranus |
0.56 |
|
|
Neptune |
0.51 |
|
|
Pluto |
0.5 |
|
ALBEDO
An object's albedo is the ratio of the amount of solar radiation
reflected from an object to the total amount it receives. An
object with a high albedo is shinier than an object with a low
albedo. A white, completely reflecting object has an albedo of
1.0; a black object with no reflectivity has an albedo of 0.0
(zero).
|
|

ALBIREO
Albireo (beta Cygni) is a third magnitude star in the
constellation called
Cygnus (Albireo is the head of the swan and the
second-brightest star in Cygnus). Albireo is a
double star; the primary (Albireo A, a K3II bright giant) is
bright yellow and the companion (Albireo B) is blue. Albireo is
roughly 386 ± 26 light years from us. |

ALDEBARAN
Aldebaran is the brightest star in the
constellation Taurus (it is one of the bull's eyes) and is the
13th brightest star in the sky. Aldebaran is seen along the
ecliptic. Aldebaran means "the Follower" in Arabic (since it
seems to follow the stars in the
Pleiades. Aldebaran is an giant, old, orange star that is
cooler than the Sun; it is under 4,000 Kelvin (the Sun is 5,800
Kelvin). Aldebaran is about 40 times as big as the Sun. |
ALDRIN, EDWIN E., JR.
 Edwin
Eugene Aldrin, Jr. (1930- ) was the second man to walk on the
moon. Also known as "Buzz" or "Dr. Rendezvous," Aldrin was the
Lunar Module Pilot (July 16-24, 1969) on NASA's Apollo 11 mission.
He and Neil Armstrong (the first man on the moon) were on the moon
for about 2 hours, collecting rock samples and doing lunar surface
experiments. Aldrin's first space mission was Gemini 12, which
launched on November 11, 1966; he and Command Pilot James Lovell
orbited Earth for 4 days. Aldrin has written many books about his
life and his career as an astronaut. |

ALGOL
Algol (Beta Persei) is a star in the
constellation Perseus. Algol was the first known
eclipsing binary star. It has a magnitude that ranges from 2.1
to 3.4; the period is 2.9 days. |
|

ALNITAK
Alnitak (Zeta Orionis) is a star at the eastern end of the
Orion's belt (in the
constellation Orion). Alnitak means belt. Alnitak is spectral
Type O9.7Ib. It is also known as Alnitah. The other two stars in
Orion's belt are Alnilam and
Mintaka. |
ALPHA
Alpha is the first letter in the Greek alphabet. Alpha often
denotes the brightest star in a
constellation.
|
ALPHA CENTAURI
Alpha Centauri is the star system that is closest to the Earth.
The dimmest star in the system, Proxima Centauri (Alpha Centauri
C), is the closest star to us (other than our sun). The stars
Alpha Centauri A and Alpha Centauri B are close binary stars. |
ALMUCANTAR
An almucantar (also called a "parallel of altitude") is a circle
on the celestial sphere that is parallel to the horizon. It
consists of all points at a given altitude - if two points are on
the same almucantar, they have the same altitude. |
ALTAIR
Altair (alpha Aqu) is a fist-magnitude star in the (in the
constellation Aquila (the eagle); Altair is the 12th brightest
star in the sky. Altair means "flying eagle" in Arabic. Altair is
in the Summer Triangle, which it forms with
Vega and
Deneb. |

ALTITUDE
Altitude is a measurement in mapping astronomical objects on the
celestial sphere (the sky as visible from Earth). Altitude is the
angle of the object from the observer's horizon. If an object is
on the horizon, its altitude is 0 degrees. If it is at the
observer's zenith, its altitude os 90 degrees. To find an object
in the sky, two coordinates are needed, its
azimuth and its altitude. |

ALT-AZIMUTH TELESCOPE MOUNT
An Alt-Azimuth telescope mount is a "U"-shaped device that allows
the telescope to move both up and down (Altitude) and left to
right (Azimuth). |

ALVAREZ THEORY OF EXTINCTION
This theory is that a large
asteroid,
meteor, or
comet hit the Earth 65 million years ago, causing huge
atmospheric and geologic disruptions, leading to a
mass extinction which killed the
dinosaurs and many other species. |
ALVAREZ, LUIS
Luis Alvarez (1911-1988) was a physicist who, with his son Walter
Alvarez (a geologist), hypothesized that the a huge asteroid hit
Earth the Earth 65 million years ago, causing a mass extinction.
The
Alvarez Theory of Extinction is widely accepted. Luis Alvarez
received a Nobel Prize in physics (1968) for his work on subatomic
particles. |

AMALTHEA
Amalthea (J-V) is the third-closest moon of Jupiter and the
largest of
Jupiter's smaller moons. It is a small, red, elongated,
cratered moon (with two very large craters); it has the fastest
speed of any known moon. It is potato-shaped, with dimensions: 145
x 91 x 83 miles (232 x146 x134 km). Its mass is 7.17x1021kg.
Amalthea's mean distance from Jupiter is 181,300 miles. It takes
Amalthea about 12 hours to orbit Jupiter; like most of Jupiter's
moons, it is in
synchronous orbit. It was discovered and named in 1892 by the
American
astronomer Edward Emerson
Barnard. |
AMOR ASTEROID
Amors are
asteroids which orbit between the orbits of Earth and Mars.
They were named for the asteroid Amor, #1221. Eros (#433) is an
Amor asteroid. |

ANALEMMA
The analemma is a figure-8-shaped diagram that shows the
declination of the sun (the angle that the sun is from the
equator), for each day in the year. If you took a snapshot of the
the sun at the same time each day (from the same location), the
Sun would make a figure shaped like an analemma in a year (this is
because the Earth is tilted on its axis and because it doesn't
orbit the Sun in a perfect circle). |
ANANKE
Ananke is
Jupiter's thirteenth moon. Ananke is 12.5 miles (20 km) in
diameter and orbits 13,100,000 miles (21,200,000 km) from
Jupiter. Ananke has a mass of 4 x 1016kg.
It orbits Jupiter in 631 (Earth) days and is in a retrograde orbit
(orbiting opposite to the direction that Jupiter rotates). Very
little is known about Ananke. Ananke was discovered by S.
Nicholson in 1951. |

ANDROMEDA
Andromeda (the princess, the daughter of Cassiopeia in mythology)
is a northern hemisphere
constellation. Alpha Andromedae (called Sirrah, meaning
"Horse's navel") is the same as Delta Pegasi (from the
constellation
Pegasus). |

ANDROMEDA GALAXY
The Andromeda Galaxy (also known as M31 and NGC 224) is the
closest major
galaxy. It is a
spiral galaxy (like
our galaxy) and is in the
Local Group. It can just be seen with the naked eye in the
constellation
Andromeda. |
ANGSTROM
An Angstrom is equal to one ten billionth (1 x 10-10)
of a meter. This unit of measure is named for the Swedish
physicist Anders J. Ångström. |
ANGULAR DISTANCE
Angular distance is the measure of an arc (a segment of the
circumference of a circle). Angular distance measures the
proportion of a circle that the arc in question consists of.
Angular distance is expressed in
degrees, radians, arc minutes (one-sixtieth of a degree), or
arc seconds (one-sixtieth of a minute). For example, latitude is
the angular distance north or south of the equator measured in
degrees, and longitude is the angular distance east or west of the
prime meridian (which goes through Greenwich, England), measured
in degrees. |
ANGULAR MOMENTUM
Angular momentum is a momentum-like quantity associated with a
circular motion around an
axis of rotation. Essentially, it is the amount of spin an
object has. Formally, Angular momentum = mass x velocity x radius
(from point that the object is spinning or orbiting around).
Angular momentum is conserved (in the absence of an outside
force). |
|
ANISOTROPY
Anisotropy is a state in which a physical characteristic
(like the temperature of the cosmic background radiation) varies
in value along axes in different directions - a physical
measurement made in one direction differs from the measurement
made in another direction. For example, the cosmic microwave
background radiation (the radiant heat left over from the Big
Bang) is anisotropic. |

ANNULAR ECLIPSE
An annular eclipse is a type of
solar eclipse. During an annular
eclipse, the
Sun looks like an "annulus" or ring. The ring is visible when
the Moon does not entirely cover the disc of the Sun during the
eclipse. This type of eclipse happens when the Sun is at
perihelion (closest to the Earth, making the solar disc appear
larger) and the Moon is at
apogee (farthest from the Earth, making it look smaller). |
ANORTHOSITE
Anorthosite is a type of rock found on the moon, on lunar
highlands. Anorthosite is composed of aluminum and calcium
silicates. |

ANTARES
(Alpha Scorpii) Antares (meaning "Rival of Mars") is the brightest
star in
Scorpius, one of the
constellations in the
zodiac. Antares is a M1.5Iab variable red supergiant star that
is about 520 light-years from Earth and is about 230 times as big
as the
Sun. This incredibly massive, old, low-temperature (3500 K)
star is the 15th brightest star in the sky; it has a visual
(apparent) magnitude of +0.96 (var.) and an absolute magnitude of
-5.2. |

ANTENNA
An antenna (plural antennae) is a conductor that can transmit or
receive radio waves. Radio telescopes are antennae (or a series of
antennae). |
ANTIMATTER
Antimatter is matter that is composed of the counterparts of
ordinary matter. For example, positrons are the antimatter
counterpart of electrons; positrons have a positive charge instead
of a negative charge. The existence of an antimatter version of
the electron was predicted by Paul Dirac in 1930. Carl Anderson,
in 1932, found positron tracks that were produced by cosmic rays
in a cloud chamber. Antimatter is also produced in some
radioactive decays. A particle and its antimatter particle will
annihilate when they meet, and energy is released (according to
Einstein's E = mc2).
Antiparticles have the same mass as their counterpart, but the
opposite charge. There seems to be very little antimatter in the
universe. |
|
ANTIPODAL POINT
A point that is on the opposite side of a celestial body from a
given point is an antipodal point. For example, the North and
South Poles are antipodal points on the Earth. |

APASTRON
The apastron is the point of greatest separation of two stars, as
in a binary star system orbit. |
|

APERTURE
The aperture is the size of a
telescope's main lens (or mirror). |

APHELION
For an object (a planet or comet) orbiting the
Sun, the aphelion is the point in its orbit which is farthest
from the sun. |

APOAPSIS
For an object orbiting a celestial body, the apoapsis is the point
in its orbit which is farthest from that body. |

APOGEE
For an object orbiting the Earth, the apogee is the point in its
orbit which is farthest from the Earth. |
APOLLO OBJECT or APOLLO ASTEROID
Apollo asteroids have an orbit that crosses the orbit of the Earth
and have a period longer than 1 year. They have a semimajor axes
greater than 1 astronomical unit (au), and perihelion distances
less than 1.017 au. These asteroids were named for asteroid
Apollo, #1862. Geographos is an Apollo. |

APOLLO MISSIONS
NASA's Apollo missions (1961 to 1975) were the only missions to
send people to the
moon. Apollo 11's LEM or LM (Lunar Excursion Module or Lunar
Module) landed on the moon on July 20, 1969. Apollo 12 to 17
continued lunar exploration. |

APOLLO 11
NASA's Apollo 11 (1969) was the first mission to send people to
the
moon. The spacecraft launched from Cape Kennedy, Florida, USA,
on July 16, 1969, from the Kennedy Space Center Launch Complex
39A. Apollo 11's LEM or LM (Lunar Excursion Module or Lunar
Module, dubbed the Eagle) separated from the orbiter and landed on
the moon on July 20, 1969, with Neil Armstrong and Buzz Aldrin.
Michael Collins was in the command-service module (CSM), the
orbiter (which was dubbed the Columbia). The LM landed at the Mare
Tranquillitatis (Sea of Tranquility). Armstrong and Aldrin were on
the moon's surface for 21 hours, 38 minutes, 21 seconds. They took
off in the LM and rendezvoused with the command-service module (CSM);
the Descent stage of the LM remained on Moon, at the Sea of
Tranquillity landing site. Apollo 11 landed in the Pacific Ocean
on July 24, 1969. The ship carried 21.7 kilograms of Moon rocks
back to the Earth. The command module "Columbia" is on display at
the National Air and Space Museum in the Milestones of Flight
gallery, Washington, D.C., USA. |
| Star |
Absolute Magnitude |
Apparent Magnitude |
Distance from Earth
(light-years) |
|
The Sun |
+4.8 |
-26.72 |
0.000016 |
| Sirius |
+1.4 |
-1.46 |
8.6 |
| Canopus |
-2.5 |
-0.72 |
74 |
| Rigel Kentaurus |
+4.4 |
-0.27 |
4.3 |
| Arcturus |
+0.2 |
-0.04 |
34 |
| Vega |
+0.6 |
0.03 |
25 |
| Capella |
+0.4 |
+0.08 |
41 |
|
Rigel |
-8.1 |
+0.12 |
900 |
| Betelgeuse |
-7.2 |
+0.7 |
1,500 |
| Altair |
+2.3 |
+0.77 |
16 |
|
Deneb |
-7.2 |
+1.25 |
1,500 |
|
Proxima Centauri |
+15.5 |
+11.05 (var.) |
4.3 |
APPARENT MAGNITUDE
Apparent magnitude is a measure of the brightness of a celestial
object as seen from
Earth. The lower the number, the brighter the object. Negative
numbers indicate extreme brightness. The full
moon has an apparent magnitude of -12.6; the sun's is -26.8.
We can see objects up to 6th magnitude without a telescope.
Apparent magnitude is abbreviated m. This system of rating the
brightness of celestial objects was developed by the Greek
astronomer
Hipparchus in 120 B.C.
|
APPARENT MOTION
Apparent motion is the observed motion of astronomical obejcts
from Earth. The apparent motion might be due to the movement of
the object or themovement of the Earth. For example, the apparent
motion of a star is caused only by the motion of the
Earth (and not by the motion of the star). |
APPARENT TIME
Apparent time is the local time, determined by the angle of the
sun. |
APPARENT SOLAR DAY
An apparent solar day is the period of time between two successive
passages of the sun across a
meridian. |

AQUARIUS
[Abbreviation: Aqr] Aquarius (the water bearer), abbreviated Aqr,
is a
constellation of the
zodiac. This faint constellation is seen along the
ecliptic. The sun passes through Aquarius from mid-February
until mid-March. There are many interesting celestial objects in
this large constellation, including
globular clusters (M2 and M72),
planetary nebulae (NGC 7009 and NGC 7293), the star group M73,
a double star (zeta Aqr). Aquarius is the
radiant for the
meteor showers: March Aquarids, Delta Aquarids, Eta Aquarids,
and Iota Aquarids. Alpha Aquarii (the brightest star in Aquarius)
is called Sadalmelik (meaning the Lucky One of the King) and beta
Aquarii (the second-brightest star in Aquarius) is named Sadalsuud
(meaning the Luckiest of the Lucky); they are twin supergiants. |
ARACHNOIDS
Arachnoids are round networks of fractures in Venus' crust. They
are called arachnoids because they loook a bit like spider webs
(spiders are
arachnids). |
ARC
An arc is a segment along the circumference of a circle. |
ARC MINUTE
An arc minute is a measure of angularity and is equal to
one-sixtieth of a degree (there are 360 degrees in a circle). |
ARC SECOND
An arc second is equal to one-sixtieth of an arc-minute. |

ARCTURUS
(Alpha Boötis) Arcturus is the brightest star in the
constellation
Boötes (the herdsman). It is a red giant (spectral type
K1.5IIIp) that is the fourth brightest star in the sky. Arcturus
is 34 light-years from Earth. It has an apparent magnitude of
-0.04 and an absolute magnitude of 0.2. |
ARECIBO DISH
The Arecibo Dish is the world's largest
radio telescope. The 1,000 ft (305 m) dish is built into a
natural hollow in the hills of Puerto Rico. |

ARIEL
Ariel is the brightest and one of the largest of the 18 moons of
Uranus. It is a moon with many long rift valleys, canyons, and
craters. It has a diameter of 720 miles (1158 km) and orbits
Uranus at a mean distance of 120,000 miles (190,930 km). It
revolves around Uranus in 50.5 Earth hours. Its mass is 1.27x1021
kg. It was discovered in 1851 by
William Lassel, an amateur English
astronomer. |

ARIES
[Abbreviation: Ari] Aries (the ram) is a constellation of the
zodiac located along the ecliptic between Pisces and Taurus.
This tiny, faint constellation is seen just north of the
ecliptic. The brightest star in Aries (Alpha Ari) is Hamal,
the second-brightest star (Beta Ari) is Sharatan, the
third-brightest star (Gamma 2 Ari) is Mesarthim, and the
fourth-brightest is Botein (Delta Ari) |

ARISTARCHUS
Aristarchus of Sámos (310?BC-250?BC) was an ancient Greek
astronomer who was the first person to propose a heliocentric
model of the Solar System. Aristarchus realized that the Earth
rotates on its axis and revolves around the Sun. He estimated how
far the Sun and the moon are from the Earth and how big the Moon
and the Sun are. Archimedes and Plutarch wrote of Aristarchus'
works. He also calculated a relatively precise value for the
length of the solar year. Aristarchus invented a bowl-shaped
sundial whose pointer cast shadows in the middle of the bowl. A
lunar crater was named for Aristarchus (pictured above); it is
located on the NW edge of the Oceanus Procellarum. This huge,
circular crater is 25 miles (40 km) in diameter and 2.2 miles (3.6
km) deep (from rim to floor). |

ARISTOTLE
Aristotle (384-322 BC) was a Greek philosopher who theorized about
astronomy. Using only philosophical speculation (he did no
scientific observations), Aristotle believed that the universe is
spherical, finite, and centered around the Earth. Aristotle, like
many others of his time, believed that the circle was the
"perfect" shape, so the universe must be spherical, and all the
orbits in it must also be circular. He also believed that
celestial bodies were composed of ether (in addition to the four
other basic elements believed to exist at that time, earth, air,
fire, water). Aristotle's ideas were adopted by the Church and
were not tested for over a thousand years, until
Galileo's experiments demonstrated errors in Aristotle's
writings. |

ARMILLARY SPHERE
An armillary sphere is an instrument from the 1500s that was used
to determine the relative positions of the
celestial equator, the
ecliptic, the planetary orbits, etc. This device consisted of
a series of concentric rings. |
ARMSTRONG, NEIL
 Neil
Alden Armstrong (1930- ) was the first person to walk on the
moon. He piloted NASA's Apollo 11 mission, which took off on
July 16, 1969. Armstrong and Edwin E. (Buzz) Aldrin, Jr., landed
on the moon on July 20, 1969, in the lunar module (landing in the
Mare Tranquilitatis), while Michael Collins orbited the moon in
the command module. Upon his first step on the moon, Armstrong
said, "One small step for man, one giant leap for mankind."
Armstrong and Aldrin explored the Moon's surface for about 2
hours. Years earlier, in 1966, Armstrong and David R. Scott
performed the first successful docking of two vehicles in space on
the Gemini 8 mission. |
D'ARREST, H.L.
Heinrich Louis d'Arrest (1822-1875) was a Danish
astronomer and the co-discoverer of
Neptune (in 1846), with
Galle. |

ASTERISM
An asterism is a collection of stars (within a
constellation) that forms an apparent pattern from Earth. Some
familiar asterisms include the
Big Dipper, the
Little Dipper,
Pleiades,
Trapezium, and the
Summer Triangle. |

| Asteroid Name and Number |
Diameter
(km) |
Mass
(kg) |
Discoverer, Date of Discovery |
| 1. Ceres |
960 x 932 |
8.7x1020 |
Piazzi, 1801 |
| 2. Pallas |
570 x 525 x 482 |
3.18x1020 |
Heinrich Olbers, 1802 |
| 3. Juno |
240 |
2.0x1019 |
K. Harding, 1804 |
| 4. Vesta |
530 |
3.0x1020 |
H. Olbers, 1807 |
ASTEROID
An asteroid is a large rocky object or very small planet
(planetoid). Most asteroids orbit the Sun in the asteroid belt
between
Mars and
Jupiter. A few asteroids approach the
Sun more closely. An asteroid impact with the Earth may have
caused the
extinction of the
dinosaurs. The largest asteroid and first one ever discovered
(by
Giuseppe Piazzi on January 1, 1801) is Ceres, whose mass is
equal to over one-third of the 2.3 x 1021
kg estimated total mass of all the 3,000 catalogued asteroids. |

ASTEROID BELT
The asteroid belt is a doughnut-shaped concentration of
asteroids orbiting the Sun between the orbits of Mars and
Jupiter (2.2 - 3.3 A.U.). This belt may have once been a planet
(in the same orbit) that was destroyed by a collision with a huge
asteroid or
comet. |
ASTHENOSPHERE
The asthenosphere is a part of the upper mantle that exhibits
plastic (flowing) properties. It is located below the lithosphere
(the crust and rigid upper mantle), between about 100 and 250
kilometers deep. |
ASTROBIOLOGY
Astrobiology is the
science that addresses the question of whether or not there is
life in space, and if so, then what it its origin, distribution,
and evolution. |
ASTROLABE
An
astrolabe is an instrument that was used to determine the
altitude of objects (like the sun) in the sky. It was first used
around 200 B.C. by astronomers in Greece. The astrolabe was
replaced by the sextant. |
ASTROMETRY
Astrometry is the precise measurement of the position and motion
of astronomical objects, often with respect to standard star
catalogues. |

ASTRONAUT
Astronauts are people who go into space. |

ASTRONAUTICS
Astronautics is the science of the design, construction, and
operation of spacecraft. |

ASTRONOMER
An astronomer is someone who studies astronomy. |
ASTRONOMER ROYAL
The Astronomer Royal is appointed by the Queen (or King) of
England to be custodian of the Greenwich Observatory. The first
Astronomer Royal, John Flamsteed, was appointed in 1675 by King
Charles II . |

ASTRONOMICAL UNIT
An astronomical unit, or AU, is equal to the mean (average)
distance from the Earth to the
Sun, about 93 million miles (150 million km). It takes a beam
of light about 8.3 minutes to travel 1 AU. |
ASTRONOMIC SCINTILLATION
Atmospheric scintillation is the twinkling of stars (fluctuation
of intensity) seen through a planet's atmosphere. Scintillation in
caused when the star's light is distorted by the
Earth's atmosphere. Scintillation is greater for bright stars
that are low on the horizon. It is also known as stellar
scintillation. |
ASTRONOMY
Astronomy is the scientific study of space, including the
planets,
stars, galaxies,
comets, and
nebulae. |

NASA'S ASTRONOMY PICTURE OF THE DAY |
ASTROPHYSICS
Astrophysics is a branch of astronomy that studies the physical
properties of celestial bodies and other matter and energy in
space. |

ASYMPTOTIC GIANT BRANCH
The Asymptotic Giant Branch is the upper right hand corner of the Hertzsprung-Russell (H-R) diagram that represents stars in which
Helium burning no longer occurs in their cores - red giants. As
the carbon core of these old star collapses, the outer layers
expand, and the star becomes huge red giants. |
ATEN ASTEROID
Atens are asteroids that are always closer to the Sun than the
Earth is; they have a period shorter than 1 year (the semi-major
axis is smaller than Earth's). They were named for asteroid Aten,
#2062. Ra-Shalom is an Aten asteroid. |
|

ATLAS
Atlas is one of the smallest of the
18 moons of Saturn. Atlas is a
shepherd satellite for Saturn's A-ring. It has a radius of
about 18.5x17.2x13.5 km. Atlas orbits at about 137,670 km from
Saturn. Its orbital period is 0.6019 earth days. It was
discovered by R. Terrile/Voyager 1 in 1980.
|

ATMOSPHERE
The atmosphere is the mixture of gases that surrounds a planetary
object, moon or star. The
Earth's atmosphere is mostly nitrogen; the
Sun's atmosphere is mostly
hydrogen gas. |

ATOM
All matter is made up of tiny atoms. An atom is the smallest part
of an element that has the properties of that element. Atoms
consist of a nucleus (containing
protons and
neutrons) and orbiting
electrons. |

ATOMIC NUMBER
An atom's atomic number of an element is the number of protons in
the nucleus of one of its atoms. The atomic number indicates the
place of an element in the periodic table of the elements. |
|

ATOMIC WEIGHT
An atom's atomic weight measures the total of the mass of the
protons, neutrons, and
electrons. The atomic weight is roughly equal to the number of
protons and
neutrons, with only a little bit added by the mass of the
electrons. |
AU
|
Planet |
Distance from the Sun
(measured in
AU) |
|
Mercury |
0.39 |
|
Venus |
0.723 |
|
Earth |
1.0 |
|
Mars |
1.524 |
|
Jupiter |
5.203 |
|
Saturn |
9.539 |
|
Uranus |
19.18 |
|
Neptune |
30.06 |
|
Pluto |
39.53 |
AU
AU stands for "astronomical unit." An AU is equal to the mean
(average) distance from the Earth to the sun, about 93 million
miles (150 million km = 500 light-seconds). |
|

AURORA
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. |
AUTUMNAL EQUINOX
Equinoxes are days in which daytime and nighttime are of equal
duration. The two yearly equinoxes occur when the
Sun crosses the
celestial equator. The autumnal equinox occurs around
September 21; the vernal (spring) equinox occurs around March 21.
|
Axial Tilt
| Planet |
Axial Tilt
(Obliquity to the Ecliptic) |
|
Mercury |
2° |
|
Venus |
2° |
|
Earth |
23.45° |
|
Mars |
24° |
|
Jupiter |
3.1° |
|
Saturn |
26.7° |
|
Uranus |
97.9° |
|
Neptune |
28.8° |
|
Pluto |
57.5° |
AXIAL TILT
Axial tilt, or obliquity to the ecliptic, is the tilt of a
planet's axis from perpendicular to the plane of the ecliptic.
Another way of looking at it is the angle between the plane of the
planet's orbit and that of the equator.
|
|

AXIS
An axis is an imaginary straight line around which an object, like
a planet, turns. The Earth's axis is a line that goes through the
North and South Poles. |

AZIMUTH
Azimuth is a measurement in mapping astronomical objects on the
celestial sphere (the sky as visible from Earth). Azimuth is the
angle of the object from the observer's north point (projected
onto the
horizon). If an object is due north, its azimuth is 0 degrees.
If it is due east, its azimuth is 90 degrees, etc. To find an
object in the sky, two coordinates are needed, its
altitude and its azimuth.
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