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PALLAS
Pallas is the second-biggest asteroid and one of the four
brightest asteroids. Its dimensions are: 570 x 525 x 482 km and
its mass is 3.18 x 1020 kg. Pallas is about 4.145 x
108 km from the Sun and takes 4.61 years to orbit the
Sun once (Pallas' year). Pallas was discovered by Heinrich
Olbers in 1802. |
PALOMAR OBSERVATORY
Palomar Mountain Observatory is an astronomical observatory
located on Palomar Mountain in southern California, USA. It has
a 200-in. (508-cm) reflecting telescope and a 48-in. (122-cm)
Schmidt telescope. It was founded by the astronomer George E.
Hale. |
PAN
Pan is one of the smaller of the many moons of Saturn. Pan is
located within the Encke Gap in Saturn's rings. Pan has a radius
of about 10 km. Pan orbits at 133,583 km from Saturn. Its
orbital period is 0.575 earth days. Pan was discovered by Mark
R. Showalter/Voyager 2 in 1990. |

PANDORA
Pandora is one of the smaller of the 18 moons of Saturn. Pandora
is a shepherd satellite for the outer edge of Saturn's F Ring.
It has a radius of about 55x44x31 km. Pandora orbits at 141,700
km from Saturn. Its orbital period is 0.62 earth days. Pandora
was discovered by S. A. Collins and D. Carlson/Voyager 1 in
1980. |

PANGAEA
(pronounced pan-JEE-ah) Pangaea was a supercontinent consisting
of all of Earth's land masses. It existed during the Permian
period through the Jurassic period. It began breaking up during
the Jurassic period, forming the continents Gondwanaland (South
America, Africa, India, Australia, and Antarctica) and Laurasia
(North America, Europe, Asia, Greenland, and Iceland). |

PARABOLA
A parabola is a conic section, a curve that is a set of points
(P) such that the distance from a line (the directrix) to P is
equal to the distance from P to focus F. Parabolas have an
eccentricity of 1. |
PARALLACTIC MOTION
parallactic motion is the apparent motion of the stars that is
caused only by the motion of the Earth as it orbits the Sun. |

PARALLAX
Parallax is the apparent change in the position of a star that
is caused only by the motion of the Earth as it orbits the Sun.
Friedrich Wilhelm Bessel first detected the parallax "motion" of
a star in 1838 observing the star 61 Cygni (this was definitive
proof that the Earth orbits the Sun, and not the other way
around). |

PARKES TELESCOPE
Parkes Telescope is a 64 meter radiotelescope in New South
Wales, Australia. |
PARSEC
A parsec is a unit of distance that is equal to 3.26 light-years
or 3.085678 x1013kilometers. It is the distance at
which a star would have a parallax of 1 second of arc. |
PARTIAL ECLIPSE
A partial eclipse happens when the moon partially blocks the sun
or the Earth's shadow partially blocks our view of the moon. |
PASIPHAE
Pasiphae is Jupiter's fifteenth moon. Pasiphae is 22 miles (36
km) in diameter and orbits 14,600,000 miles (23,500,000 km) from
Jupiter. Pasiphae has a mass of 2 x 1023kg. It orbits
Jupiter in 735 (Earth) days and is in a retrograde orbit
(orbiting opposite to the direction of Jupiter). Very little is
known about Pasiphae. Pasiphae was discovered by P. Melotte in
1908. |
PATERA
A patera is shallow crater with a complex, scalloped edge. |
PAYLOAD
The payload is the cargo carried on the Space Shuttle or other
spacecraft. |
PECULIAR GALAXY
A peculiar galaxy is an irregular galaxy that has an abnormal
shape (neither elliptical, spiral, nor lenticular) and/or has
another unusual characteristic, like jets of gas spewing from
the nucleus, unusual amounts of dust, low surface brightness,
etc. They are probably formed as galaxies collide or have
companion galaxies that influence them. Peculiar galaxies are
generally smaller and optically dimmer than regular galaxies.
They have the designation p or pec at the end of
their name. In 1966, the astronomer Halton Arp published a
catalogue of 338 of these galaxies in his "Atlas of Peculiar
Galaxies." Arp suggested that peculiar galaxies create stars in
intense bursts. Ring galaxies are a type of peculiar galaxy. |

PEGASUS
Pegasus (the flying horse) is a large northern hemisphere
constellation. Delta Pegasi is shared with the constellation
Andromeda. 51 Pegasi (51 Peg), off the Great Square of Pegasus,
is a nearby, Sun-like star that has been found to have an
orbiting planet. |

PENUMBRA
The penumbra is the outer, relatively light region of a sunspot
shaped like an annulus (ring) surrounding the darker, cooler
umbra. |

PENUMBRA
The penumbra is the area of partial shadow (compare to umbra). |

PERIGEE
For an object orbiting the Earth, the perigee is the point in
each orbit which is closest to the Earth. The perigee varies a
small amount from orbit to orbit. The closest perigee is called
the proxigee. |

PERIHELION
The perihelion is a planet or comet's closest approach to the
Sun. The Earth is at perihelion (the Earth is closest to the
Sun) in January. |
PERIOD OF REVOLUTION
The period of revolution of an orbiting body is the time it
takes for it to make one revolution around its primary body. The
period of revolution for the Earth is one year. |

PERIOD OF ROTATION
The period of rotation of an orbiting body is the time it takes
for it to make one rotation around its axis. The period of
rotation for the Earth is one day. |

PERMIAN PERIOD
The Permian period preceded the Triassic period, when dinosaurs
and mammals evolved. It lasted from 280 to 248 million years
ago. |

PERSEID METEOR SHOWER
The Perseids are a meteor shower that occur each year from July
23-Aug. 22, with a maximum on Aug. 12. This meteor shower occurs
each year as the Earth passes through the orbit of the comet
Swift-Tuttle, and icy remnants of the comet burn up as they
enter the Earth's atmosphere. This meteor shower has am average
magnitude of 2.3. The meteors in this shower seem to emanate
from the constellation Perseus (but they do not). |

PERSEUS
Perseus is a constellation in the Milky Way in the Northen
Hemisphere. It is abbreviated Per. Perseus' major star is alpha
Per, called Marfak or Algenib; it is an F5 supergiant. Beta Per
is the eclipsing binary Algol. Perseus was a hero in Greek
mythology who killed the monstrous Medusa. Each year in August,
the Perseid meteor shower radiates from this constellation's
northern part. |
PERTURBATION
A perturbation of the orbit of a planet or a satellite causes it
to deviate from a simple, theoretically regular elliptical
orbit. Orbital perturbations are caused by other celestial
bodies (like nearby planets) exerting gravitational forces on
the orbiter. Orbital perturbations can lead to exciting
discoveries; Pluto was discovered because Uranus and Neptune had
orbits that were known to be perturbed by some unknown object. |

PHASES OF MATTER
Matter can exist in four phases (solid, liquid, gas, and plasma)
and a few other extreme phases, like critical fluids and
degenerate gases. The phase diagram of water (above) shows its
phase at various temperatures and pressures. |

PHASES OF THE MOON
As the moon circles the Earth, the shape of the moon appears to
change; this is because different amounts of the illuminated
part of the moon are facing us. The shape varies from a full
moon (when the Earth is between the Sun and the moon) to a new
moon (when the moon is between the sun and the Earth). The
phases of the Moon include: the new moon, waxing crescent, first
quarter, waxing gibbous, full moon, waning gibbous, last
quarter, waning crescent, and new moon again. |

PHOBOS
Phobos (meaning "fear") is the larger of the two tiny moons of
Mars. It is only 13.8 miles (22.2 km) across and has a mass of
1.08x1016. It orbits Mars at a mean distance of 5,600
miles (9,000 km). Its major feature is a large crater, named
Stickney (Hall's wife's maiden name), which is 6.2 miles (10 km)
wide. Phobos may be a captured asteroid. Phobos was discovered
by A. Hall in 1877. |

PHOEBE
Phoebe is one of the smaller of the 18 moons of Saturn. Phoebe
has an almost circular shape and a reddish color. It rotates on
its axis every 9 hours, unlike the other moons of Saturn (except
Hyperion) which always show the same face to Saturn. It has a
radius of about 110 km and mass of 4 x 10 18kg.
Phoebe orbits at 12,952,000 km from Saturn. Its orbital period
is 550.48 earth days. Phoebe was discovered by W. Pickering in
1898. |
PHOTOELECTRIC EFFECT
The photoelectric effect is a phenomenon in which electrons are
ejected from a the surface of a metal when light shines on the
metal. Albert Einstein explined the photoelectric effect in
1921. |

PHOTOEVAPORATION
Photoevaporation is a phenomenon in which the intense light from
hot stars causes gases to evaporate (boil away) into
interstellar space. In the Eagle Nebula (pictured above),
ultraviolet light boils off some of the hydrogen gas (H2),
continually re-shaping the columns of the nebula. |
PHOTOMETRY
Photometry is the measurement of apparent magnitudes of
astronomical objects, like stars. |
PHOTON
A photon is a quantum of electromagnetic energy. For example,
light is composed of light. |

PHOTOSPHERE
The photosphere is the layer of the Sun which is visible to us.
It consists of a plasma and has a temperature of about 10,800°F
(6,000°C). |

PIAZZI, GIUSEPPE
Giuseppe Piazzi (1746-1826) was an Italian astronomer who
discovered and named the first (and largest) asteroid, Ceres, on
January 1, 1801. Asteroids are large, rocky objects that orbit
the Sun in a belt between Mars and Jupiter. |
PIONEER 10
Pioneer 10/11 were early NASA missions to explore the Solar
System and beyond. Pioneer 10 was launched in 1972 and went to
Jupiter. 29 years later, in 2001, signals were received from
Pioneer 10 - it was over 7 billion miles from Earth heading
towards the star Aldebaran (in the constellation Taurus). |
PIONEER 11
Pioneer 10/11 were early NASA missions to explore the Solar
System and beyond. Pioneer 11 launched in 1973, travelling to
Jupiter, heading toward the constellation of Aquila. The last
transmission from Pioneer 11 was received in 1995. |

PISCES
[Abbreviation: Psc] Pisces (the fish) is a faint equatorial
constellation of the zodiac. Pisces is seen along the ecliptic
between Aries and Aquarius. The brightest star in Pisces (Alpha
Psc) is Al Rischa (or Alrisha), the second-brightest-star (Beta
Psc) is Fum al Samakah. The spiral galaxy M74 is in Pisces. |

PISTOL STAR
The Pistol star is the largest-known star; it is the most
massive and the brightest star. It is 10 million times brighter
than our Sun and 100 times more massive. This star is at the
center of the Pistol Nebula and created it by expelling
tremendous amounts of gas in violent eruptions. |
PLANE OF THE ECLIPTIC
The plane of the ecliptic is the plane of our solar system. In
the course of a year, the sun traces a path in the sky along the
ecliptic. The Earth's axis is tilted at a 23.5° from the
ecliptic (which causes the seasons). |

PLANET
A planet is a large celestial body that orbits a star and does
not shine on its own. There are nine planets orbiting the sun in
our solar system. |

PLANETARIUM
A planetarium is a room in which images of the stars, planets,
and other celestial bodies are projected. |
PLANETARY ALIGNMENT
Planetary alignment is when many of the planets in the solar
system are roughly in a line. A large planetary alignment
occured on May 5, 2000, when Mercury, Venus, Earth, Mars,
Jupiter, and Saturn will be (very roughly) lined up, with all
the planets on the other side of the Earth from us. Also, the
Moon was almost between the Earth and Sun. This type of
alignment happens every few hundred years and has little or no
significance. |

PLANETARY NEBULA
A planetary nebula is a nebula formed from by a shell of gas
which was ejected from a certain kind of extremely hot star. As
the giant star explodes, the core of the star is exposed.
Planetary nebulae have nothing to do with planets. The Hourglass
Nebula is a planetary nebula. |
PLANETESIMAL
A planetesimal is a small object that orbits the Sun.
Planetesimals are thought to have formed when the Solar System
itself formed, and they were perhaps the building blocks from
which the planets were built. |
PLANETESIMAL HYPOTHESIS
The planetesimal hypothesis is a theory about the formation fo
the Solar System. It was proposed by Thomas Chrowder Chamberlain
(Sept. 25, 1843 - Nov. 15, 1928), an American geologist and
teacher. In this theory, a star is supposed to have passed near
the Sun, pulling matter away from the Sun. Later, this matter is
to have condensed into larger masses, forming the planets. |

PLANETOID
A planetoid is a very small planet. The larger asteroids are
sometimes called planetoids. |
PLANETOLOGIST
A planetologist is an astronomer who studies the physical
features of planets.
|
PLANETOLOGY
Planetology is a branch of astronomy that studies planets. |

PLANET SYMBOLS
Each of the planets in our Solar System has been given a symbol;
the symbols are pictured above. |

PLANET "X"
Planet "X" was the temporary name given to the then-unknown
planet beyond Neptune that disturbed the orbits of Uranus and
Neptune. Percival Lowell calculated the rough location of Planet
"X's" orbit, but died in 1916 before it was found. This planet
was eventually found by C. Tombaugh in 1930 and named Pluto).
Planet "X" is also the name given to any as-yet-undiscovered
tenth planet. There may be another Planet "X" beyond Pluto (see
Nemesis). |
PLANITA
A planita is a low plain on a planet's surface. |
PLANUM
A planum is a high plain (a plateau) on a planet's surface. |
PLASMA
A plasma is an extremely hot gas that is composed of
free-floating ions (atomic nuclei stripped of some electrons -
making the ions positively charged) and free electrons
(negatively charged). A plasma behaves much differently than a
neutral gas, and is considered the fourth state of matter. A
plasma conducts electrical currents. Stars are composed of
plasma. |

PLATES
The crust of the Earth is broken into plates. The plates are
enormous chunks of rock that float atop the soft mantle. The
plates are moving at a speed that has been estimated at 1 to 10
cm per year. Oceanic plates (those that are under the ocean) are
thinner and denser than continental plates. |
PLATE TECTONICS
Plate tectonics is the now-established theory that chunks of the
Earth's crust (plates) float on the surface and change both
position and size over time.
|

PLEIADES
The Pleiades (M45), also known as the "Seven Sisters" (and
"Subaru" in Japan), is the brightest open cluster of stars in
the sky. It is located in the constellation Taurus. Six of the
stars in the Pleiades are visible without a telescope. Roughly
500 stars belong to the Pleiades star cluster; most of these are
faint. A reflection nebula surrounds the stars. |
PLUTINO
A Plutino (meaning "little Pluto") is a main Kuiper belt
objects, ones that have a 2:3 resonance with Neptune (as Pluto
is); a 2:3 resonace means that the Plutino completes 2 orbits
around the Sun in the same time that it takes Neptune to
complete 3 orbits around the Sun. About one-quarter of the
Kuiper Belt objects (also called transneptunian objects) are
Plutinos. Compare with cubewano. |

PLUTO
Pluto is the ninth and (usually) the farthest planet from the
Sun. It has a highly inclined orbit. This small, cold, rocky
planet has one moon, Charon. |

POLARIS
Polaris (alpha UMi) is the current pole star for the Northern
Hemisphere; it is 1 degree from the exact Northern celestial
pole. In 1780, Sir William Herschel discovered that Polaris was
a double star with a faint companion star. Polaris is a
blue-green Cepheid variable star (its size brightness changes
periodically, with period of 3.969778 days; it varyies between
mag 1.92 and 2.07). Polaris has a relatively dim companion star
(9th magnitude). Polaris' distance from Earth has been estimated
to be from 360 to 820 light years. At its brightest, Polairs is
about 6,000 to 10,000 times brighter than our Sun. It is the
larger star at the end of the handle of the Little Dipper (Ursa
Minor). Polaris is also called the Lodestar or the Cynosure. |
POLAR SCOPE
A polar scope is a small telescope that is used for aligning a
larger telescope with the North or South pole star. |

POLE STAR
A pole star is a star that is located almost due north or due
south and is useful for navigation. Polaris is the pole star of
the Northern Hemisphere. |
POLIAKOV, VALERI
Valeri V. Poliakov is a Russian physician and cosmonaut who
broke many space endurance records, and holds the second-longest
record for being in space: 678 days over two flights (Sergei
Avdeyev beat his record in 1999, having been in space for 758
days). Dr. Poliakov holds the record for the single longest stay
in space, 437 days, 17 hours, 58 minutes. Poliakov was on the
Russian space station MIR missions Soyuz TM6 and TM7 (240 days,
22 hours, 26 minutes in 1988), and Soyuz TM18 (437 days, 17
hours, 58 minutes in 1994-1995). |
POPULATION 1 STARS
Population 1 stars are relatively young stars. They are found
mainly in the disk of galaxies. |
POPULATION 2 STARS
Population 2 stars are relatively old stars. They are found
mainly in the halo of galaxies. |

PORE
A pore is a small sunspot that doesn't have a penumbra. Pores
are up to about 1,500 miles (2,500 km) across and are lighter
than a sunspot's umbra. |
POSITRON
A positron (also called the positive electron or the
antielectron) is an elementary particle; it is the antiparticle
of the electron. It has the same mass and spin as an electron,
but has a positive charge (equal in magnitude to the charge of
an electron). |
PRECESSION
Precession is the small wobbling motion around the Earth's axis
that the Earth makes as it spins (just like the wobblin.g motion
of a spinning top). This causes the Earth's axis to point in a
slightly different direction over time; Polaris is our pole star
now, but this is not permanent because of precession. Precession
is caused by the gravitational influences of the Sun and the
Moon and has a period of 25,800 years. |

PRECIPITATION
Precipitation is rain, sleet, hail, snow, or other condensation
products falling from the atmosphere. Precipitation on Earth is
is key in the water cycle. Precipitation on Venus is sulphuric
acid rain. |

PRIMARY
A primary is a planetary body around which a moon or satellite
orbits. |
PRIME VERTICAL
The prime vertical is a great circle on the celestial sphere
that passes through the zenith. It is a vertical circle that is
bisected by the meridian. Degrees run from east to west. |
PROBE
A probe is an unmanned spacecraft that is sent to collect data
from space. Some probes return to Earth, others are not meant
to. |
PROCYON
Procyon (also called Alpha Canis Minoris, Antecanis, and the
Little Dog Star) is the brightest star in the constellation
Canis Minor and the eighth brightest star in the sky. This
yellowish star is also part of the Winter Triangle. Procyon is a
relatively close star; it is only about 11.4 light years from
us. Procyon is about as seven times more luminous than our
Sun.This sub-giant star is near the end of its life; it's
hydrogen core is almost spent (it has been converted into
helium). Procyon has a companion, a bersly-visible white dwarf
called Procyon B (it is only about the size of the Earth and is
about 14.9 astronomical units from Proycon A), and this small
star makes Procyon wobble from our perspective. The existence of
Procyon B was predicted in 1840 by Arthur Julius Georg Friedrich
von Auswers (1838-1915) but wasn't seen until 1896 (by John M.
Schaeberle (1853-1924)). |

PROMETHEUS
Prometheus is one of the smaller of the 18 moons of Saturn.
Prometheus is a shepherd satellite for the inner edge of
Saturn's F Ring. It has a radius of about 74x50x34 km.
Prometheus orbits at 139,353 km from Saturn. Its orbital period
is 0.613 earth days. Prometheus was discovered by S. A. Collins
and D. Carlson/Voyager 1 in 1980. |
PROMINENCE
A solar prominence is an cloud-like arc of gas that erupts from
the surface of the Sun. Prominences can loop hundreds of
thousands of miles into space. |
PROPER MOTION
Proper motion is the actual motion of a star across the sky (not
toward or away from the Earth). This motion is due to the orbit
of the star in the Milky Way Galaxy. The proper motions of a
star is the distance that it moves across the sky each year.
This distance is so tiny, that it is measured in arcseconds per
year. The star with the most proper motion is Barnard's Star
(the star system second-closest to us), which moves only10
arcseconds per year (1/180 of the apparent width of the full
moon). |
PROPLYDS
Proplyds (short for protoplanetary disks) are disks of dust and
gas in space that surround newborn stars. They appear as fuzzy
blobs, even when seen through the Hubble Space Telescope.
Proplyds may be very young solar system, consisting of a
rotating disk of gas that will eventually coalesce into a solar
system. |

PROTEUS
Proteus is the second-largest moon of Neptune. It was discovered
using NASA's Voyager 2 mission in 1989. It orbits 117,650 km
from the center of Neptune and is about 218 x 208 x 201 km in
size. This dark moon has a circular orbit just over the
cloud-tops of Neptune. Proteus is dotted with impact craters and
is irregularly shaped |
PROTOPLANETARY DISK
A protoplanetary disk is a rotating disk of dust that surrounds
the central core of a developing solar system. This disk
eventually coalesces into planets that orbit the star (which
forms from the central core). |

PROTON
Protons are small, positively-charged atomic particles. In an
atom, protons are in the nucleus, surrounded by electrons.
Protons have a mass similar to the neutron. The proton was
discovered by Rutherford in 1919 (after the discovery of the
electron and before the discovery of the neutron). |
PROTON-PROTON CHAIN
The proton-proton chain is a hypothetical fusion reaction
thought to occur deep inside stars. This chain reaction converts
hydrogen nuclei into helium nuclei and releases energy
(particles) and gamma-rays. This thermonuclear reaction is
thought to take on the order of a billion years to complete, and
occurs under tremendously high pressure and temperature. |
PROTOSTAR
A protostar is a star that is still forming and nuclear fusion
has not yet begun. |
PROTOSUN
A protosun is a star that is still forming, during the early
stages of a solar system. The protosun is the central material,
which will eventually become a sun (a star), when nuclear fusion
begins. |
PROVISIONAL NAME
A provisional name is a temporary name gicen to an object, like
a newly-discovered asteroid or a moon. |

PROXIGEAN SPRING TIDE
The Proxigean Spring Tide (also called the proxigean tide) is a
rare, unusually high tide. This very high tide occurs when the
moon is both unusually close to the Earth (at its closest
perigee, called the proxigee) and in the New Moon phase (when
the Moon is between the Sun and the Earth). The proxigean spring
tide occurs at most once every 1.5 years. |

PROXIGEE
For an object orbiting the Earth, the proxigee is the closest
perigee. The perigee is the point in each elliptical orbit which
is closest to the Earth, but the perigee varies a small amount
from orbit to orbit. |
PROXIMA CENTAURI
The closest star to us is the Sun. Other than that, the closest
star is Proxima Centauri, aka Alpha Centauri C (the dimmest star
in the Alpha centauri system). Proxima Centauri is about 4.2
light-years from the Sun. It has an absolute magnitude of 15.5
and an apparent magnitude of +11.05 (variable). Spectral type
M5.5Vc. |

PTOLEMY
Claudius Ptolemaeus or Ptolemy (about 87-150) was a Greek
astronomer and mathematician who wrote about his belief that all
celestial bodies revolved around the Earth. His writings
influenced people's ideas about the universe for over a thousand
years, until the Copernican System (with a heliocentric solar
system) was accepted. |

PTOLEMAIC SYSTEM
The Ptolemaic System is an outdated view of the solar system
written about by Ptolemy (about 87-150) in his major work,
Almagest (Mathematical Syntaxis). Ptolemy believed
that all the planets and the sun orbited around the Earth in the
order: Mercury, Venus, the Sun, Mars, Jupiter, and Saturn. He
also devised a system of circular orbits within orbits (called
epicycles) to explain the way the planets orbited around the
Earth. It was not until the 1500's when the Copernican System
(with a heliocentric solar system) was accepted. |

PUCK
Puck is one of the 18 moons of Uranus. Its diameter is about 96
miles (154 km) and its mass is unknown. It orbits at a distance
of about 53,500 miles (86,010 km) from Uranus. Puck was
discovered by NASA's Voyager 2 in 1985. |
PULSAR
A pulsar is a rapidly spinning neutron star that emits energy in
pulses. Pulsars were discovered in 1967 by S. Jocelyn Bell
Burnell (1943- ), who was a Cambridge University astronomy
graduate student at the time. Her graduate advisor (Anthony
Hewish) was given a share of the 1974 Nobel Prize, but Bell was
ignored. No one had any idea what these unusual objects were at
the time, so the name little green men (LGM) was used. Soon,
Thomas Gold suggested that pulsars were rapidly-spinning neutron
stars, the remnants of a supernova. |

PYTHAGORAS
Pythagoras of Samos (569-475 BC) was a Greek philosopher,
mathematician, and astronomer who founded a philosophical and
religious school, the Pythagorean school in Croton, Italy.
Pythagoras believed that the Earth was a sphere at the center of
the Universe. He correctly realized that the morning star and
the evening star were the same object, the planet Venus.
Pythagoras (or the Pythagoreans) made a number of fundamental
mathematical discoveries: that for a right triangle, the sum of
the squares of the two shorter sides is equal to the square of
the hypotenuse (known as the Pythagorean theorem); that the sum
of the angles of a triangle is equal to two right angles; and
that irrational numbers exist. A 142 km wide lunar crater was
named for Pythagoras (Latitude 63.5°, Longitude 63.0°). |
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