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H
H is an asteroid's absolute magnitude, the visual magnitude the
asteroid would have if it were located 1 AU from Earth. |

HADLEY, JOHN H.
John Hadley (1682-1744) was an English mathematician and
inventor who built the first reflecting telescope and invented
an improved quadrant (known as Hadley's quadrant). |

HADLEY RILLE
Hadley Rille is a long valley on the surface of the moon. This
rille is 75 miles (125 km) long, 1300 feet (400 m) deep, and
almost 1 mile (1500 m) wide at its widest point. It was formed
by molten basaltic lava that carved out a steep channel along
the base of the Apennine Front (which was explored by the Apollo
15 astronauts in 1971). |
HALE-BOPP COMET
Hale Bopp (designated C/1995 O1) is a periodic comet (made of
frozen gas and dust), that orbits around the sun. Its
earliest-recorded sighting was on July 23, 1995. It was
independently discovered by Alan Hale (of New Mexico) and Thomas
Bopp (of Arizona), both amateur astronomers. This comet has a
diameter of about 40 km; it's rotation rate is 11.4 hours. It
was last seen in 1997 and will be seen next in the year 4377;
its period is 2380 years. |
HALE, GEORGE E.
George Ellery Hale (June 9, 1868 - February 21, 1938) was an
astronomer who founded the Yerkes Observatory (1892), the Mt.
Wilson Observatory (in 1904), and the Palomar Observatory. Hale
invented the spectroheliograph (a device used to analyse the
Sun's spectrum) when he was an undergraduate at the
Massachusetts Institute of Technology (Cambridge, Massachusetts,
USA). Later, Hale discovered that sunspots were low-temperature
areas on the sun and that they had high magnetic fields. |

HALF-LIFE
The half-life of a radioisotope is the amount of time it takes
for half of the radioisotope to decay. |

HALF MOON
A half moon looks like half a circle. It is sometimes called a
quarter moon (this moon has completed one quarter of an orbit
around the Earth from its full or new position, and one quarter
of the moon's surface is visible from Earth). |
HALL, ASAPH
Asaph Hall (1829-1907) was an American astronomer who discovered
Mars' two moons, Phobos and Deimos, on August 12, 1877, at the
U. S. Naval Observatory's 26-inch refracting telescope. Angelina
Hall (nee Stickney), Hall's former mathematics professor and his
wife, helped him in his work. |
HALLEY, EDMUND
Edmund Halley (1656-1742) was an English astronomer who
predicted the return of a spectacular comet in 1758 (after his
death, this was confirmed by Johann G. Palitzsch). This comet
had previously been seen in 1531, 1607, and 1682. This comet is
now known as Halley's Comet. In 1716, Edmond Halley published a
paper describing how a planetary transit (a transit of Venus or
Mercury) could be used to measure our distance from the Sun. |

HALLEY'S COMET
Halley's comet is a periodic comet (made of frozen gas and
dust), that orbits around the sun. Its earliest-recorded
sighting was in 240 B.C. in China, but Edmund Halley was the
first person to recognize that it was periodic. It was last seen
in 1986 and will be seen next in the year 2061; its period is 76
years. When the Earth passes through Halley's comet's orbit
(twice each year), its detritus causes the meteor showers the
Eta Aquarids and the Orionids. |
HALO
A halo is a luminous ring that is sometimes seen surrounding the
sun or the moon. Some parts of the halo are very bright, others
are not very bright. Sometimes, only a part of the ring is
visible. The halo is produced as light is reflected and
refracted through tiny, flat ice crystals in the atmosphere.
Halos are always an angle of 22° away from the sun or moon, due
to the hexagonal structure of the ice crystals. The diameter of
the halo is about an eighth of the sky. |
HARTMANN, JOHANNES F.
Johannes Franz Hartmann (1865-1936) was a German astrophysicist
who, in 1904, discovered clouds of interstellar calcium gas (he
detected the absorption lines of ionized calcium atoms using
spectrography while studying binary stars). He also developed a
theory about novas, studied the asteroid #433 (Eros) and
developed a method of testing telescope lenses, which is still
named for him. |

HARVEST MOON
The Harvest moon is the full moon that appears closest in time
to the Autumnal Equinox, occurring in late September or early
October. |
HAWKING, STEPHEN
Stephen Hawking (1942- ) is a British physicist and cosmologist.
His work centers on the physics of black holes and singularities
in space-time. Hawking (1971) proposed that early after the Big
Bang, mini-black holes existed, obeying quantum-mechanical laws
due to their sub-atomic size. Hawking (1974) hypothesized that
black holes emit subatomic particles until they explode. |
HAYASHI CONTRACTION
Hayashi contraction is a gravitational phemonenon in which a
protostar becomes smaller, coalescing into a main seqence star. |
HAYASHI TRACK
Hayashi track is a phase in the life cycle of a star in which
its luminosity decreases but he surface temperature remains the
same and the star enters the main seqence in the H-R diagram. |
HD NUMBER
The HD (Henry Draper) number is an identifying number assigned
to the strs in the Henry Draper catalog. In this system, every
star is classified by its stellar spectrum. This sytem is named
for the astronomer Henry Draper, but was cataloged by Annie J.
Cannon (225,300 stars), and later extended by Margaret W. Mayall.
For example, the star Vega is HD 172167 (the spectral type is
not in the HD number). |
HEAVENLY WATERS
Heanenly Waters is a family of 9 constellations that includes
Delphinus (the Dolphin), Columba (the Dove), Equuleus (the
Little Horse), Carina (the Keel), Puppis (the Stern), Eridanus
(the river), Pisces Austrinus (the Southern Fish), Vela (the
Sails), and Pyxis (the Mariner's Compass). |
HEAVY-METAL STAR
A heavy-metal star is an unusual type of giant star. Heavy-metal
stars include barium (Ba II) stars (a type of late giant star)
and S stars (a type of red giant). |
HEKTOR
Hektor (Asteroid 624) is the largest Trojan asteroid; it is
about about 100 km long (it is elongated). Its rotation period
is 6.9225 hours. |

HELENE
Helene is one of the smaller of the 18 moons of Saturn. Helene
has a radius of about 18x16x15 km and is irregularly shaped.
Helene orbits at about 377,400 km from Saturn, leading Dione by
60°. Its orbital period is 2.74 days. Helene was discovered by
Discovered: P. Laques & J. Lecacheus in 1980. |

HELIOCENTRIC
A Heliocentric system is one in which a sun is at the center. |

HELIOCENTRIC SYSTEM
In the heliocentric model of the solar system, all the planets
orbit around the Sun. |
HELIOPAUSE
The heliopause is the boundary of the heliosphere of the Sunin
which the solar wind's density decreases greatly (and its speed
also declines). The location of this transition region is
unknown, but must be at more than 50 AU from the Sun. |
HELIOSPHERE
The heliosphere is an area centered around the Sun over which
the effect of the solar wind extends. The heliosphere extends
beyond the orbit of Pluto. |
HELIOSPHERIC TERMINATION SHOCK
The heliospheric termination shock is the shock that occurs as
the solar wind hits the heliopause and its speed slows greatly
(down to about 20 km/s). |
HELIUM
Helium is an element with the atomic number 2. It has two
protons and two neutrons in its nucleus which is orbited by two
electrons. It is the second most abundant element in the
universe. It is created from hydrogen atoms in the process of
nuclear fusion that occurs within stars. The Sun is about 25%
Helium. Helium was named after the Sun (called "Helios" in
Greek) because it was first discovered on the Sun by Jules
Janssen in 1868. Helium is plentiful on the Sun and rare on
Earth. |
HELIUM BURNING
Helium burning is a stage in a star's life in which the star
fuses helium into carbon and oxygen (through nuclear fusion).
Every star that began with more than half a Solar mass will
eventually burn helium. |
HELIX NEBULA
The Helix nebula (NGC 7293) is a planetary nebula that has the
largest angular diameter of any known planetary nebula. It is
about 140 parsecs away, in Aquarius. |
HELMHOLTZ CONTRACTION
The Helmholtz contraction is the gravitational collapse of a
protostellar cloud that is slowed by outward gas pressure and
the limited rate at which radiation can escape. |

HELMHOLTZ, HERMANN VON
Hermann Ludwig Ferdinand von Helmholtz (1821-1894) was a German
astrophysicist who studied solar energy production and star
formation. See Helmholtz contraction. |

HEMISPHERE
A hemisphere is half of a sphere. |
HENRY DRAPER CATALOG
The Henry Draper catalog is a catalog of stars in which every
star is classified by its stellar spectrum. This sytem is named
for the astronomer Henry Draper, but was cataloged by Annie J.
Cannon (225,300 stars), and later extended by Margaret W. Mayall.
For example, the star Vega is HD 172167 (the spectral type is
not in the HD number). |

HERCULES
Hercules is a Northern Hemisphere constellation that is the
fifth largest in the sky. It is named for Hercules, the
legendary hero of Greek mythology. The brightest of its rather
dim stars is Ras Algethi (alpha Her), a variable red supergiant.
The four stars of the central trapezoid within Hercules, epsilon
Her, zeta Her, eta Her, and pi Her, form the asterism called
Keystone. The globular star cluster M13 is located on the
western part of the Keystone. The Tau Herculid meteor shower
seems to radiate from Hercules. |

HERSCHEL, WILLIAM
Sir William Herschel (1738-1822) was a British astronomer and
organist who built an improved reflecting telescope and used it
to discover the planet Uranus (March 13, 1781) and moons of
Uranus and of Saturn. Herschel cataloged over 2500 discoveries,
mostly deepsky objects. Herschel's sister Caroline Lucretia
Herschel (1750-1848) helped him in his discoveries and
discovered many clusters and nebulae (and 8 comets) herself. |
HERTZSPRUNG, EJNAR
Ejnar Hertzsprung (1873-1967) was a Danish astronomer who,
independently of H. N. Russell, realized the relationship
between a star's temperature (color) and its brightness, and
designed a diagram illustrating this relationship in 1911, later
called the Hertzsprung-Russell Diagram. |

HERTZSPRUNG-RUSSELL DIAGRAM
The Hertzsprung -Russell (H-R) Diagram is a graph that plots
stars color (spectral type or surface temperature) vs. its
luminosity (intrinsic brightness or absolute magnitude). On it,
astronomers plot stars' color, temperature, luminosity, spectral
type, and evolutionary stage. This diagram shows that there are
3 very different types of stars:
- Most stars, including the sun, are "main sequence stars,"
fueled by nuclear fusion converting hydrogen into helium. For
these stars, the hotter they are, the brighter.
- Giants and Supergiants are above the main sequence.
- Faint white dwarfs (hot, dim stars) are below the main
sequence stars.
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HEVELIUS, JOHANNES
Johannes Hevelius (1611-1687) was a German astronomer who
published the first moon map. He also published a celestial
atlas introducing many constellations (including Canes Venatici,
Lacerta, Lynx, Sextans, etc.). |

HIGH TIDE
High tide is the time of high water. High tides occur when the
gravitational attraction of the moon causes the oceans to bulge
out in the direction of the moon. |
HIMALIA
Himalia is Jupiter's tenth moon. Himalia is 110 miles (170 km)
in diameter and orbits 7,000,000 miles (11,480,000 km) from
Jupiter. Himalia has a mass of 9.5 x 1018kg.
It orbits Jupiter in 250.5662 (Earth) days. Very little is known
about Himalia. Himalia was discovered by C. Perrine in 1904. |

HIPPARCHUS
Hipparchus (190-120 B.C.) was an ancient Greek astronomer who
compiled first-known catalogue of stars and first map of the
skies. He listed 850-1,000 stars, organized by constellation. He
noted each star's position and brightness (he rated the
brightness on a scale from 1 to 6, the brightest being 1).
Hipparchus also devised the system of epicycles, an
Earth-centered system in all celestial objects moved in perfect
circles around the Earth. He also founded trigonometry. |

HORIZON
The horizon is an imaginary circle that delimits the sky and the
Earth, or an extension of the plane of the observer (at an
altitude of 0 degrees). |

HORIZONTAL BRANCH
The horizontal branch is a part of the Hertzsprung -Russell
(H-R) diagram that represents stars that burn helium in thier
cores. These mostly large stars lie along the top of the H-R
diagram.
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HORSEHEAD NEBULA
The Horsehead Nebula is a huge cloud of dust in space that is
shaped like a horse's head. It is luminous at its edges because
it is in front of a bright emission nebula. It is located in the
constellation called Orion. |

H-R DIAGRAM
The Hertzsprung -Russell (H-R) Diagram is a graph that plots
stars color (spectral type or surface temperature) vs. its
luminosity (intrinsic brightness or absolute magnitude). On it,
astronomers plot stars' color, temperature, luminosity, spectral
type, and evolutionary stage. This diagram shows that there are
3 very different types of stars:
- Most stars, including the sun, are "main sequence stars,"
fueled by nuclear fusion converting hydrogen into helium. For
these stars, the hotter they are, the brighter.
- Giants and Super giants are above the main sequence.
- Faint white dwarfs (hot, dim stars) are below the main
sequence stars.
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HST
HST is an abbreviation for the Hubble Space Telescope, a
powerful telescope in orbit around the Earth. HST takes pictures
and spectra of objects in space without the interference of the
atmosphere (which makes telescopic images from the ground have
less detail); it transmits the pictures and spectra back to
scientists on Earth. The telescope was launched into space in
April, 1990, and was repaired in December, 1993. It was named
for the American astronomer Edwin Hubble. |
HUBBLE CONSTANT
The Hubble Constant, H0 is the
number (not actually a constant) which shows the rate at which
the universe is expanding. It determines the relationship
between how far a galaxy is from us and how fast it is receding
from us (because of the expansion of the Universe). H0
is between 50 and 100 km/s/mparsec. Hubble's constant can be
used to estimate the size and age of the Universe (Hubble Time).
It was formulated by E. P. Hubble in 1925. |
HUBBLE, EDWIN P.
Edwin Powell Hubble (1889-1953) was an American astronomer who
was very influential in modern cosmology. He showed that other
galaxies (besides the Milky Way) existed and observed that the
universe is expanding (since the light from almost all other
galaxies is red-shifted). |
HUBBLE'S LAW
Hubble's Law is a linear relationship between the distance to a
galaxy (R) and the velocity at which that galaxy is moving from
us (v) because to the expansion of the universe. Hubble's Law is
is v = H0 R, where H0
is Hubble's constant. It assumes that the universe is expanding
at a constant rate that has reemained constant for all time. |

HUBBLE SPACE TELESCOPE
The Hubble Space Telescope (or HST) is a powerful telescope in
orbit around the Earth. HST transmits pictures and spectra of
objects in space without the interference of the atmosphere
(which makes telescopic images from the ground have less
detail). It was launched into space in April 1990 and was
repaired in December, 1993. It was named for the American
astronomer Edwin Hubble. |
HUBBLE TIME
Hubble Time is an estimate of the age of the universe; it is the
inverse of the Hubble constant. |
HUGGINS, WILLIAM and MARGARET
Sir William Huggins (February 7, 1824-May 12, 1910) was an
amateur English astronomer who was the first person to use
spectroscopy to determine the compositions of astronomical
objects (in 1861). He determined that the Sun and the stars are
composed mostly of the element hydrogen. He also examined the
spectra of nebulae and comets. Huggins' wife (they were married
in 1875), Margaret Lindsay Murray Huggins (1848-1915), was a
self-taught astronomer who did extensive work in spectroscopy
and photography. Margaret studied the Orion Nebula extensively.
William and Margaret were the first people to realize that some
nebulae, like the Orion Nebula, consisted of amorphous gases
(and were not a congregation of stars, like the nebula
Andromeda). A lunar crater, a Martian crater, and an asteroid
(#2635 Huggins) have been named for William Huggins. |

HUYGENS, CHRISTIAN
Christian Huygens (1629-1695) was a Dutch physicist and
astronomer who developed new methods for grinding and polishing
glass telescope lenses (about 1654). With his new, powerful
telescopes, he identified Saturn's rings and discovered Titan,
the largest moon of Saturn in 1655. Huygens also invented the
pendulum clock in 1656 (eliminating springs), wrote the first
work on the calculus of probability (De Ratiociniis in Ludo
Aleae, 1655), and proposed the wave theory of light (Traité de
la lumiere, 1678). |
HYDROGEN
Hydrogen is the element with the atomic number 1. It is the
lightest element and the most abundant in the universe. Its
nucleus is a single proton which is orbited by one electron. It
fuels nuclear fusion that occurs within stars, converting
hydrogen into helium. The sun is 75% hydrogen. |

HYDROLOGIC CYCLE
The Hydrologic Cycle (also known as the water cycle) is the
journey water takes as it circulates from the Earth to the sky
and back again. |
HYDROPONICS
Hydroponics is a method of growing plants in water that contains
dissolved nutrients (instead of in soi). |
HYDROSTATIC EQUILIBRIUM
Hydrostatic equilibrium is a stable condition in a star in which
the fluid matter within the star is at an equilibrium with
respect to all forces, including the inward-pulling force of
gravity, the out-ward pulling buoyancy due to pressure
differentials, and the out-ward pulling forces of radiative
pressure. |
HYPATIA
Hypatia of Alexandria (AD 370(?)-415) was a Greek mathematician,
astronomer, teacher, and head of the Platonist school at
Alexandria about AD 400. Hypatia wrote commentaries on the
astronomical canon of Ptolemy and did work on conic sections .
Her works are lost, but are referred to in the Suda lexicon. She
was the daughter of the mathematician and philosopher Theon of
Alexandria (he was also the last head of the Museum at
Alexandria). A pagan, she was murdered in 415 by Christian monks
in a religious/political struggle. The lunar Crater Hypatia and
Rimae Hypatia were named for her. |

HYPERBOLA
A hyperbola is a conic section (the intersection of a cone with
a plane) that has two mirror-image branches. Hyperbolas have an
eccentricity greater than 1. |

HYPERBOLIC ORBIT
A hyperbolic orbit is an orbit in which the eccentricity is
greater than 1. |

HYPERION
Hyperion is one of the 18 moons of Saturn. Hyperion is the
largest-known irregular-shaped body in our Solar System. It has
a variable rotational period. Craters mark the surface. Iapetus
has a radius of about 180x140x112.5 km and is irregularly
shaped. Hyperion orbits at about 1,481,100 km from Saturn. Its
orbital period is 21.27 days. It was discovered by W. & G.
Bond/W. Lassell in 1848. |
HYPERNOVA
A hypernova is an enormous collapse and subsequent explosion of
a supergiant star that eventually forms a black hole. This
explosion is bigger than a supernova and is accompanied by a
gamma-ray burst. The plural of hypernova is Hypernovae. |
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