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M# (MESSIER OBJECTS)
During the late 18th century (1759-1781), the French
astronomer Charles Messier made a list of 103 fuzzy objects
in space in order not to mistake star clusters, galaxies, and
nebulae for comets (for which he was searching). More objects
were added later, bringing the total to 110. In it, M1 is the
Crab Nebula, M2 is a globular cluster in Aquarius, M3 is a
globular cluster in Canes Venatici, etc. For a list of the
Messier objects, click here. |

M31
M31 (commonly known as Andromeda Galaxy) is the closest major
galaxy to us. It is a
spiral galaxy (like our galaxy, the
Milky Way). It can just be seen with the naked eye. |
MACHO
MACHO stands for Massive Compact Halo Object. MACHOs are objects
that could account for some (or all) of the dark matter in the
halos of galaxies, like white dwarfs, neutron stars, and black
holes. |

MAGELLANIC CLOUDS
The Magellanic Clouds are irregular-shaped
galaxies, congregations of millions of stars. The irregular
shape may be the result of a disturbance, perhaps a collision of
two galaxies. The Large Magellanic Cloud (LMC) is near the
constellation Dorado, and is 163,000
light-years away. The Small Magellanic Cloud (SMC) is near
the constellation Tucana, and is under 200,000 light-years away.
These two clouds are satellites of our
Milky Way Galaxy. |

MAGMA
Magma is molten rock (lava) from which igneous rock forms.
|
MAGNETAR
A magnetar is a highly magnetic star. Magnetar have magnetic
fields of about 1015 Gauss,
about a thousand trillion times stronger than the
Earth's. The strong magnetic field puts the star's surface
under enormous stress, perhaps causing "starquakes"
and resulting high energy bursts of radiation. These short-lived
neutron stars were theorized to exist in 1992 by Robert C.
Duncan and Christopher Thompson. Their existence was confirmed
in 1998 by Chryssa Kouveliotou et al. |
|
Magnetic Field Size |
|
The Earth at the equator |
0.32 Gauss |
|
The Earth at the poles |
0.62 Gauss |
|
Refrigerator magnets |
102 Gauss |
|
Sunspots |
103 Gauss |
|
Fields produced in
labs |
105 Gauss |
|
Magnetars |
8 x 1014 Gauss |
MAGNETIC FIELD
A
magnetic field is a region near a magnet where other magnets are
affected. The
Earth's magnetic field is probably caused by its molten
iron-nickel core. This field is aligned with the north and south
poles, and has reversed many times during geologic history.
William Gilbert hypothesized that the Earth was a giant magnet
in 1600. |
MAGNETIC STORM
A magnetic storm is a temporary perturbation (disruption) of the
Earth's magnetic field, caused by
solar flares, which eject plasma from the
Sun's chromosphere. This solar plasma travels at speeds of
roughly 600 to 1,200 miles per second (1,000 to 2,000 km per
second), and after about 21 hours, hit the Earth's atmosphere.
Since they disturb the
ionosphere (the upper atmosphere), magnetic storms can
disrupt radio transmissions. Magnetic storms usually last for a
few days. During a magnetic storm,
auroras increase over polar regions.
|
|
MAGNETOPAUSE
A magnetopause is the boundary between the area in which a
planet's magnetic field dominates and the magnetic field of the
rest of the Solar System dominates.
|

MAGNETOSPHERE
The
magnetosphere is the Earth's magnetic environment. The Earth
is a huge dipole (2-pole) magnet. The Earth's magnetic field is
probably cause by its molten iron-nickel core. This magnetic
field is aligned with the north and south poles, and has
reversed many times during geologic history. Charged particles
become trapped on the field lines of the magnetosphere. William
Gilbert hypothesized that the Earth was a giant magnet in 1600.
Thomas Gold proposed the name "magnetosphere" in 1959. The
Earth's magnetosphere extends far into space and is influenced
by the solar wind (ions and electrons emitted from the sun). It
extends into space from 60 to 37,280 miles (100 to 60,000 km)
towards the Sun, and over 186,500 miles (300,000 km) away from
the Sun, forming the Earth's magnetotail. |
| Star |
Absolute Magnitude |
Apparent Magnitude |
Distance from Earth
(light-years) |
|
The Sun |
+4.8 |
-26.72 |
. |
| 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 |
MAGNITUDE
Magnitude is a measure of brightness of celestial objects. Lower
numbers represent brighter objects than higher numbers; very
bright star are 1st magnitude, less bright stars are 2nd
magnitude, etc. The magnitude scale is logarithmic; a difference
in magnitude of 5 is a 100-fold increase in brightness (the
difference in each successive magnitude is a factor of about
2.512 times). This system of rating the brightness of celestial
objects was developed by the Greek astronomer Hipparchus in 120
B.C. The current system was developed in 1850 by the English
astronomer Norman Robert Pogson.
Apparent magnitude is the visible brightness of an object
from Earth. Absolute magnitude is the brightness the object
would have if seen from a distance of 10 parsecs (32.6
light-years) from Earth. Bolometric magnitude includes a star's
entire spectrum of radiation, not just the visible light. |

MAIASAURA
The
first dinosaur in space was Maiasaura peeblesorum (a
duck-billed dinosaur). A piece of bone from a baby
Maiasaura and a Maiasaura eggshell were taken into space by
astronaut Loren Acton on an 8-day NASA mission (Spacelab 2) in
1985. The historic Maiasaura fossils now reside at the Museum of
the Rockies in Bozeman, Montana, USA. |

MAIN SEQUENCE STARS
Main sequence stars are the central band of stars on the
Hertzsprung-Russell Diagram. These stars' energy comes from
nuclear fusion, as they convert Hydrogen to Helium. Most
stars are Main Sequence Stars. For these stars, the hotter they
are the brighter. The sun is a typical Main Sequence star. |

MAIN SEQUENCE TURNOFF
The main sequence turnoff is the place on the
Hertzsprung-Russell Diagram where an aging (evolving) star
begins to run out of hydrogen in the core and expand, thus
moving off the main sequence. |

MAKSUTOV-CASSEGRAIN TELESCOPE
A Maksutov-Cassegrain telescope (MCT) is a wide-angle reflecting
telescope with a curved correcting lens (called a Meniscus
Corrector Shell.) that minimizes spherical aberration and a
concave mirror that receives light and focuses an image. A
second mirror reflects the light through a gap in the primary
mirror, allowing the eyepiece or camera to be mounted at the
back end of the tube. The
Cassegrain telescope (named for the French sculptor Sieur
Guillaume Cassegrain) was developed in 1672; the Meniscus
Corrector Shell (a curved lens that corrected spherical
aberration and was easier to produce than the
Schmidt's correction lens) was added in 1941 by Dmitry
Maksutov from Russia and A. Bouwers of Holland. |
| Mariner Mission |
Planet Explored |
Date of Launch |
| Mariner 1 |
None (attempted Venus flyby) |
1962 |
| Mariner 2 |
Venus |
1962 |
| Mariner 3 |
None (attempted Mars flyby) |
1964 |
| Mariner 4 |
Mars flyby |
November 28, 1964 |
| Mariner 5 |
Venus flyby |
1969 |
| Mariner 6 |
Mars |
February 24, 1969 |
| Mariner 7 |
Mars |
March 27, 1969 |
| Mariner 8 |
None (attempted Mars orbiter) |
1971 |
| Mariner 9 |
Mars orbiter |
May 30, 1971 |
| Mariner 10 |
Venus/Mercury flyby |
1973 |
MARINER
NASA's series of Mariner misisons were designed to gather
information from the planets
Venus,
Mercury, and
Mars. They were sent to map these planets and take
atmospheric measurements (like temperature, composition,
pressure, and density).
|

MARIUS, SIMON
Simon (Mayr) Marius (1570-1624), was a German
astronomer and physician who studied with
Kepler and attended Galileo's lectures. He claimed to have
discovered the four largest
moons of Jupiter in 1610, the same year that
Galileo discovered them (independently). |

MARS
Mars, the "red planet," is the fourth planet from the sun. |

MARS FACE
This photograph of the Cydonia Mense region of
Mars was taken by NASA's Mars Global Surveyor in 1998. It is
a coincidental alignment of rocks and other geologic formations
that happens to look like a human face from this angle. |
| Planet |
Mass
(kg) |
|
Mercury |
3.3 x1023 |
|
Venus |
4.87 x1024 |
|
Earth |
5.98 x1024 |
|
Mars |
6.42 x1023 |
|
Jupiter |
1.90 x1027 |
|
Saturn |
5.69 x1026 |
|
Uranus |
8.68 x1025 |
|
Neptune |
1.02 x1026 |
|
Pluto |
1.29 x1022 |
MASS
Mass is a measure of the quantity of matter.
|
MASS DEFECT
The mass of an atomic nucleus is less than the sum of the masses
of the individual protons and
neutrons that constitute it. This difference in mass is
called the mass defect. When protons and neutrons come together
to form an atomic nucleus, the extra mass is converted into
energy (E=mc2), which is
released. Stars are powered by this mechanism. |
MASS EXTINCTION
Mass extinction is the process in which huge numbers of species
die out suddenly. The dinosaurs (and many other species) went
extinct during the
K-T extinction, which was probably caused by an asteroid
colliding with the Earth. |
MASS LUMINOSITY RELATION
The mass luminosity relation states that more massive a star is,
the more luminous it is. |
MATTER
Physical objects are made of matter. Matter can exis3t in four
phases (solid,
liquid,
gas, and
plasma) and a few other extreme phases, like
critical fluids and
degenerate gases. |
|

MCAULIFFE, CHRISTA
Sharon Christa Corrigan McAuliffe (1948-1986) was an American
schoolteacher who chosen to be first teacher in space. She was
killed, along with her six fellow astronauts (Francis R. Scobee,
Michael J. Smith, Judith A. Resnik, Ellison S. Onizuka, Ronald
E. McNair, and Gregory B. Jarvis), when the NASA's Space Shuttle
Challenger Mission 51-L exploded only 73 seconds after its
launch on the morning of January 28, 1986. McAuliffe was born on
September 2, 1948, in Boston, Massachusetts. She taught at
Concord High School in New Hampshire before being chosen for the
Space Shuttle mission (she was chosen from over 11,000
applicants). McAuliffe was married and had two children. |
MEGAPARSEC
A megaparsec (Mpc) is a unit of distance that is equal to one
million
parsecs, 3.26 x 106
light-years or 3.085678 x1019
kilometers. The
Local Group of galaxies is roughly a megaparsec in diameter.
|

MERCURY
Mercury is the planet closest to the sun. It a small, dense,
rocky planet with almost no atmosphere. |
MERIDIAN
The meridian is an imaginary north-south line in the sky that
passes through the observer's
zenith. |
|
MESON
Mesons are a type of hadron (strongly interacting particles)
that contain an even number of quarks. Most mesons are composed
of one quark and one antiquark. Examples include the pion,
B-meson and the kaon.
|

MESOSPHERE
The mesosphere is the atmospheric layer between the
stratosphere and the
ionosphere. The mesosphere is characterized by temperatures
that quickly decrease as height increases. The mesosphere
extends from between 31 and 50 miles (17 to 80 kilometers) above
the earth's surface. |
MESSIER, CHARLES
Charles Messier (1730-1817), was a French
astronomer who searched the skies for comets. He compiled a
list of 103 fuzzy objects (nébuleuse sans étoile, or starless
nebulosities) in space in order not to mistake star clusters,
galaxies, and nebulae for comets (for which he was searching).
The Messier list has been added to and now consisted of 35
galaxies, 30 open clusters, 29 globular clusters, 4 planetary
nebulae, 7 diffuse nebulae, and two unconfirmed objects (which
were mistaken for nebulae by Messier). |

MESSIER OBJECTS
During the late 18th century (1759-1781), the French
astronomer Charles Messier made a list of 103 fuzzy objects
in space in order not to mistake star clusters, galaxies, and
nebulae for comets (for which he was searching). More objects
were added later, bringing the total to 110. In it, M1 is the
Crab Nebula, M2 is a globular cluster in Aquarius, M3 is a
globular cluster in Canes Venatici, etc. |

METAMORPHIC ROCK
Metamorphic rocks are compacted by pressure and heat from deep
inside the earth. |

METEOR
A meteor is a
meteoroid that has entered the Earth's atmosphere, usually
making a fiery trail as it falls. It is sometimes called a
shooting star. Most burn up before hitting the Earth. |

METEORITE
A meteorite is a meteor that has fallen to Earth. Meteorites are
either stone, iron, or stony-iron. |

METEORITES FROM MARS
Many meteorites from Mars have landed on Earth, one with a
suspected microbial fossil. |
|
| Meteor Shower |
Approximate Dates |
Date of Maximum |
Approximate Hourly Rate of Meteors |
Velocity
km/sec |
Parent Comet |
| Quadrantids (visible
by Boötes) |
Dec. 8-Jan. 7 |
Jan. 3 |
40-60 |
42 |
unknown |
| Lyrids |
Apr. 16-25 |
Apr. 22 |
10-15 |
48 |
Thatcher 18611 |
| Eta Aquarids |
April 21-May 12 |
May 5-6 |
20-50 |
66 |
Halley (periodic) |
| Delta Aquarids |
July 14-Aug.18 |
July 28-29 |
20 |
41 |
unknown |
| Perseids |
July 23-Aug. 22 |
Aug. 12 |
50-75 |
60 |
Swift-Tuttle
(periodic) |
| Orionids |
Oct. 15-29 |
Oct. 21-22 |
20-25 |
66 |
Halley (periodic) |
| Southern Taurids |
Sept 17-Nov. 27 |
Oct. 30- Nov. 7 |
10-15 |
- |
Encke (periodic) |
| Leonids |
Nov. 14-20 |
Nov. 17-18 |
15-80+++ |
71 |
Tempel-Tuttle
(periodic) |
| Geminids |
Dec. 6-19 |
Dec. 13-14 |
50-85 |
35 |
Asteroid #3200
Phaeton |
| Ursids |
Dec. 17-25 |
Dec. 22 |
15 |
34 |
Tuttle 1790 |
METEOR SHOWER
A meteor shower is a phenomenon in which many meteors fall
through the atmosphere in a relatively short time and in
approximately parallel trajectories. They occur when the Earth
passes through a
comet's orbit, and left-over comet debris (rocks, etc.)
bombards the Earth. Each meteor shower occurs at a predictable
time each year. Showers are named after the
constellation they seem to originate from (their
radiant). A huge meteor shower is called a meteor storm; it
can produce up to thousands of meteorite each hour.
|
|

METEOROID
Meteoroids are tiny stones or pieces of metal that travel
through space. |

METEOR STORM
A meteor storm is a very intense
meteor shower.
|
METHANE
Methane (CH4) is an odorless,
colorless, flammable gas.
|

METIS
Metis is the closest of
Jupiter's 16 moons . Metis is 25 miles (40 km) in diameter
and orbits 79,500 miles (128,000 km) from Jupiter, within
Jupiter's main ring. Metis and the next moon, Adrastea, are
probably the source of the dust in this ring. Metis has a mass
of 9 x 1016kg. It orbits
Jupiter in 0.294780 (Earth) days; this is faster than Jupiter
rotates on its axis. Metis was discovered by Stephen Synnott
(Voyager 2) in 1980. |
MICROGRAVITY
Microgravity is a state in which gravity is reduced to virtually
negligible levels. For example, when an object is in free fall,
it experiences microgravity. |
MICROWAVE RADIATION
Microwave radiation is a type of electromagnetic radiation that
has a wavelength between 1 mm and 30 cm. |
MILANKOVITCH THEORY
The Milankovitch Theory attempts to explain major temperatures
changes on Earth, especially ice ages, by slight variations in
the amount of sunlight reaching the Earth caused by the
eccentricity of the Earth's orbit around the Sun. The Earth's
orbital eccentricity changes the Earth's average distance from
the sun and therefore slightly changes the amount of sunlight
reaching the Earth. Milankovitch looked over the past 600,000
years and correlated summer temperature mimnima with four major
ice ages in this time. Eccentricity cycles last over 100,000
years. This theory was proposed by Milutin Milankovitch in 1938.
Recently, scientists (Richard A. Muller and Gordon J. MacDonald,
July 11, 1997, Science) have found that changes in the
axal tilt of the Earth's orbit more closely match glacial cycles
for the past million years. |

MILKY WAY
The Milky Way is a bright line of stars stretching across the
night sky. It is easier to see when you are far from bright city
lights. |

MILKY WAY GALAXY
The Milky Way Galaxy is a
spiral galaxy; our sun and
solar system are a small part of it. Most of the stars that
we can see are in the Milky Way Galaxy. The main plane of the
Milky Way looks like a faint band of white in the night sky. The
Milky Way is about 100,000 light-years in diameter and 1,000
light-years thick. There are about 2 x 10
11 stars in the Milky Way. This
spiral galaxy formed about 14 billion years ago. It takes
the sun roughly 250 million years to orbit once around the Milky
Way. The Earth is about 26,000
light-years from the center of the Milky Way
Galaxy. The major arms of the Milky Way galaxy are the
Perseus Arm, Sagittarius Arm, Centaurus Arm, and Cygnus Arm; our
Solar System is in a minor arm called the Orion Spur. |
MILLIBAR
A millibar is a unit of pressure equal to a thousandth of a
bar. |
MILLIKAN
Robert Andrews Millikan (Mar. 22, 1868-Dec. 19, 1953) was an
American physicist who measured the charge of the electron (in
his oil-drop experiment, 1911). Millikan named "cosmic rays" in
1928, while studing the radiation from space. He won the Nobel
Prize for Physics in 1923 for his work on the electron's charge
and his work on the photoelectric effect. Millikan wrote many
books. |
1,000,000
MILLION
A million is a thousand thousand. The dinosaurs lived millions
of years ago. |

MIMAS
Mimas is one of larger of the 18 moons of Saturn. It has a
diameter of 235 miles (390 km) and it orbits at about 116,000
miles from Saturn. It has a very cratered surface, including one
huge crater, Herschel, that is about one quarter of the moon's
diameter (80 miles = 130 km wide). Herschel's central mountain
is 4 miles (6 km) tall, taller than Mount Everest. Mimas has
very low temperatures (-200° C = -328°F). Its orbital period is
about 22.5 Earth days. Mimas was discovered by
William Herschel in 1789. |

MINERAL
A mineral is a naturally-occurring solid of definite chemical
composition whose atoms usually form a regular pattern. |

MINOR PLANET
A minor planet is another name for an asteroid. |

MINTAKA
Mintaka (Delta Orionis) is the uppermost and faintest of the
three major stars that form belt of Orion, a
constellation in the Northern Hemisphere (the other two
stars in the belt ate
Alnitak and Alnilam). Mintaka (which means "belt") is
located quite near the celestial equator. It is the seventh
brightest star in Orion; it is a variable star of magnitude
2.22-2.5; it is also a double star. It is about approximately
915 light-years from Earth. Its spectral type is O9.5II . |

MIR
Mir (which means "peace" in Russian) was a Russian space
station, the first semi-permanent human habitat in orbit around
the Earth. The first part of Mir (the Mir module) was launched
on February 20, 1986; it orbited the Earth for over 15 years.
Mir is composed of many of different modules that have been
attached to it through the years; the modules perform different
functions. Cosmonauts and astronauts from many countries have
lived and performed scientific experiments on Mir. Mir fell back
to Earth on March 23, 2001. |

MIRA
Mira (Omicron Ceti) is a well-known variable
red giant star in the
constellation called
Cetus. It was discovered in 1596 by David Fabricus, an
amateur Dutch
astronomer. Mira (meaning "wonderful") was named by Johannes
Hevelius in 1662. Its mass is about the same as our
Sun but it varies in size and brightness over a period of
332 days (about 11 months). During this period, its
magnitude varies from 3.4 to 9.3. |

MIRANDA
Miranda is one of the 18 moons of
Uranus. Its surface is marked by huge grooves, and appears
to have shattered many times. It has a bright, V-shaped groove
on its surface, the Inverness Corona, which has been nicknamed
the chevron. Miranda's diameter is about 290 miles (470 km) and
its mass is 6.3 x10+19 kg. It
orbits at a distance of about 80,000 miles (129,780 km) from
Uranus, and orbits once every 33.8 hours. It was discovered by
Gerard Kuiper in 1948. |
| Some Mira Variable Stars |
Magnitude Range |
Period (days) |
| R Carinae |
3.9-10.5 |
308.7 |
| R Centauri |
5.3-11.8 |
546.2 |
Mira
(Omicron Ceti) |
3.4-9.3 |
332.0 |
MIRA VARIABLE STAR
A Mira variable star is a
variable star whose brightness and size cycle over a very
long time period, in the order of many months. Miras are
pulsating
red giants that vary in magnitude as much as a factor of
many hundred (by 6 or 8 magnitudes). Mira variables were named
after the star Mira, whose variations were discovered in 1596.
|
MITCHELL, MARIA
Maria Mitchell (August 1, 1818
-June 28, 1889 ) was the first woman Professor of Astronomy of
the United States. In 1865, Maria Mitchell became a professor of
astronomy at Vassar College in Poughkeepsie, New York (she had
previously been a librarian) . She discovered a comet (in 1847),
studied the planets Jupiter and Saturn, and photographed many
stars. Despite her accomplishments, when she visited the Vatican
Observatory in Italy, she was only allowed to enter the
observatory during the day. Maria Mitchell was the first woman
accepted into the American Academy of Arts and Sciences (1848),
the Association for the Advancement of Science (1850), and the
American Philosophical Society (1869). Mitchell was one of the
founders of the American Association for the Advancement of
Women (1873). |
Mohorovicic, Andrija
Andrija Mohorovicic (1857 - 1936) was a Yugoslavian
geophysicist. After examining seismic waves from the 1909 Kulpa
Valley earthquake, Mohorovicic theorized that a boundary between
the Earth's crust and the upper mantle existed (about 50 km
beneath the surface) in which the speed of earthquake waves
became very rapid. This region is now called the Mohorovicic
discontinuity. A crater on the far side of the moon was also
named for Mohorovicic. |

MOHOROVICIC DISCONTINUITY
The Mohorovicic discontinuity separates the crust and the upper
mantle of the
Earth. |
MOLDAVITE
Moldavite is a rare, glassy, translucent, dark green gemstone.
Moldavite is a silica-based tektite, a mineral formed when a
meteorite (a rock from space) struck the Earth's surface and
melted and fused the surrounding rock. Moldavite is only found
in Bohemia (the Czech Republic) in the Ries Crater in the Moldau
River valley (which it was named for). Moldavite was discovered
in the late 1800's; the meteorite from which it formed hit the
Earth about 14.7 million years ago. Moldavite has a
Mohs hardness of 5.5-6.6. Inclusions of gas bubbles and
iron/nickel spherules are common. This natural glass has been
used for jewelry, religious articles, and decorative objects
since prehistoric times. |
MOMENTUM
Momentum is an object's mass times its velocity. |
MONOCHROMATIC
Monochromatic means having light of only one wavelength. |

MONS
A mons is a mountain. For example, the Olympus Mons is a huge
mountain (an extinct volcano) on
Mars. |

MOON
The moon is Earth's only natural satellite. It travels around
the Earth in about one month (27 days 8 hours). It is about
240,000 miles (384,000 km) from Earth. The temperature on the
Moon ranges from -320°F to 248°F (-160°C to 120°C). The moon has
no atmosphere. |

MOON BUGGY
The Moon buggy (also known as the lunar rover or the Lunar
Roving Vehicle) was a Jeep-like vehicle that the astronauts used
to drive on the
moon during the Apollo 15, 16, and 17 missions. It weighed
450 pounds, (or 75 pounds in the Moon's gravity). It could carry
1000 Earth-pounds. On the flight from the Earth to the moon, the
lunar rover was folded up in the lunar module. There are three
abandoned lunar rovers on the Moon. |

MOON LANDING
NASA's Apollo missions sent people to the
moon for the first time. Apollo 11's LEM (Lunar Excursion
Module) was the first to land on the moon, on July 20, 1969,
with
Neil Armstrong and Buzz Aldrin (Michael Collins was in the
orbiter). Apollo missions 12 through 17 continued lunar
exploration. |
MOONRISE
The
moon rises and sets every day, appearing on the horizon just
like the
sun. The time depends on the
phase of the moon. It rises about 30 to 70 minutes later
each day than the previous day, so the moon is out during
daytime as often is it's out at night. At the time of the new
moon, the moon rises at about the same time the sun rises, and
it sets at about the same time the sun sets. As the days go by
(as it waxes to become a crescent moon, a half moon, and a
gibbous moon, on the way to a full moon), the moon rises during
daytime (after the sun rises), rising later each day, and it
sets at nighttime, setting later and later each night. At the
full moon, the times of moonrise and moonset have advanced so
that the moon rises about the same time the sun sets, and the
moon sets at about the same time the sun rises. As the moon
wanes (becoming a half moon and a crescent moon, on the way to a
new moon), the moon rises during the night, after sunset, rising
later each night. It then sets in the daytime, after the sun
rises. Eventually, the moon rises so late at night that it's
actually rising around sunrise, and it's setting around sunset.
That's when it's a new moon once again. |
| Planet |
Number of Moons |
| Mercury |
0 |
| Venus |
0 |
| Earth |
1 |
| Mars |
2 |
| Jupiter |
16 |
| Saturn |
18 |
| Uranus |
15 |
| Neptune |
1 |
| Pluto |
1 |
MOONS
A moon is a large body that orbits around a planet. Many planets
have moons.
|
MOORE, PATRICK
Patrick Moore (1923- ) is an English
astronomer who has written over 60 books on astronomy and
made regular BBC television appearances popularizing astronomy.
He has done work on lunar mapping. |
MT. WILSON OBSERVATORY
The Mt. Wilson Observatory
is an astronomical observatory located in Pasadena, California,
California. It was founded in 1904 by the astronomer
George E. Hale. |
MULLER, JOHANN
Johann Müller, also known as Johann Regiomontanus (1436-1476)
was a German
astronomer and mathematician. He studied trigonometry,
translating
Ptolomy's Almagest, from the original Greek.
Ironically, his translation helped overthrow the Ptolomaic view
of the universe (in which the Earth was thought to be at the
center of the universe). He also did work on plane and spherical
trigonometry. Muller also obsesrved the motion of the moon,
planets, and comets. A 108 km diameter lunar crater, called
Regiomontanus (Latitude: -28.3 degrees, Longitude: 1.0 degrees),
was named for Muller. |
MUSES-CN
MUSES-CN is a Japanese nanorover, a small, book-sized rover
designed to be sent to explore the Near-Earth
asteroid 4660 Nereus. MUSES stands for the Mu Space
Engineering Spacecraft; C indicates that it is third in a
series, N is for NASA. It will be launched from Japan in Jan.
2002; 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). |

MUTTNIK
Muttnik is a term that many people used for the dogs who were
sent into space on
Sputnik missions. Between 1958 and 1961, the USSR (now
Russia) sent 13 dogs into space in preparation for future
missions.
Laika (meaning "barker" in Russian) was the first dog in
space; she was launched in Sputnik 2 on November 3, 1957. |
1,000,000
MYA
"mya" stands for millions of years ago. |
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