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Phobos
Phobos

... gravitational field of a foreground star amplifies the light of a background star that momentarily aligns with it. The particular character of the light magnification can reveal clues to the nature of the foreground star and any associated planets. However, without identification and characterizatio ...
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... Launched in 1989, the Galileo Spacecraft, on its way to Jupiter, captured close-up images of asteroids Gaspra and Ida. Launched in 1996, the Near Earth Asteroid Rendezvous - Shoemaker (NEAR Shoemaker), passed near asteroid 253 Mathilde and established orbit around 433 Eros. In 2001, NEAR Shoemaker “ ...
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Astrophysics Outline—Option E

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the constellations of the zodiac

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1. Estimate the average mass density of a sodium atom assuming its

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Topic Outline - Physics Rocks!

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... Pattern in the Sky • Star pattern repeats itself about every 24 hours… because of the rotation of Earth with respect to the distant stars! • Star pattern in the winter is different from that in the summer… because of the revolution of Earth around the Sun! • Stars do move back a nd forth (a teeny-ti ...
Measuring Stars
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... Since a large interstellar cloud first fragments to smaller pieces when it collapses under gravity, end result is a cluster of stars. All stars in a cluster are of the same age and composition, an ideal place to study the effect of mass on the stellar evolution. There are two main types of star clus ...
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Exam Name___________________________________

... 83) Which of the following statements is true? A) A large atom can be photographed with the aid of an ordinary microscope. B) There are only about 100 different kinds of atoms that combine to form all substances. C) An atom is the smallest particle known to exist. D) There are thousands of different ...
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Review Sheet // Study Guide: ESS Semester II 2002

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Experiment 36 – Extraterrestrial microwaves

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... They had huge differences in character, and Johannes Kepler and Ticho Brahe did not work together. Ticho Brahe feared Kepler would steal his ideas so he only showed him half of his voluminous data. Later, Ticho Brahe died first and Kepler got his data, with which he worked for 29 years until he died ...
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... Any star is so far away that, no matter where on earth you view it from, it appears to be in almost exactly the same direction. This is not necessarily the case for an object in the solar system; the moon, for instance, is only 60 earth radii away, so its direction can vary by more than a degree as ...
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... 3. A planet orbits a star at a radius of 1 AU. One orbit takes ½ of an earth year. The mass of the star is ___ the mass of the sun. ...
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... • How did we come to be? —The matter in our bodies came from the Big Bang, which produced hydrogen and helium. —All other elements were constructed from H and He in stars and then recycled into new star systems, including our solar system. • How can we know what the universe was like in the past? • ...
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... convection zone and dissipate in the solar atmosphere. Solar flares After the sunspots, another significant and most dramatic phenomenon of solar activity is solar flares, which can be defined as a sudden, rapid, and intense variation in brightness, which influence the earth strongly. On Sept.1, 185 ...
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Planetary motion - Inside Mines

... • Heliocentric model – the Sun is at the center of the Universe. Not correct either since the Universe has no center (see Cosmology), but solves the problem of the very complex motions of the planets around the Earth! • Nicolaus Copernicus (1473-1543) ...
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... A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, (c) has not cleared the neighborhood around its orbit, and (d) is not a satellite. ...
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... the brightest star in Leo. However, dazzling Jupiter one-thousandth that of the Sun, but two and a half times outshines this star by over 30 times. that of all the other planets in the Solar System combined. Jupiter is a gas giant, along with Saturn. (Uranus and Neptune are ice giants.) Jupiter was ...
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Extrasolar Planets = 403

... Planets orbiting stars other than the Sun Smaller than 13 Jupiter masses First planet around ordinary star is 51 Peg 1995 Most found using Iodine cell technique pioneered at DAO, UBC, UVic ...
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(Issue 6), June 2014

... The inner part of moon’s shadow is called Umbral shadow and the outer part is known as Unfortunately, not every eclipse of the Sun is Penumral shadow. a total eclipse. Sometimes, the Moon is too small to cover the entire Sun’s disk. It occurs Total solar eclipse occur when the Umbral part because th ...
Lecture 1a: Class overview and Early Observations 8/27
Lecture 1a: Class overview and Early Observations 8/27

... 365.242 days in year- not on tests •  If normal year has 365 days need extra 24 days/century and extra 2 days/millennium •  46 BC Julius Caesar (really Sogigula an Egyptian) - Julian calendar with leap day every 4 years. But 8 too many days every 1000 years so…. •  Gregorian calendar adopted Spain ...
Astronomy and Space Science
Astronomy and Space Science

... For the Sun, the absolute magnitude is 4.8 and luminosity is 3.83×1026W. We have M = 71.3 - 2.5 log10(L), where L is in W. More: Using this and earlier formulae, we can see how the physical quantities m, d, M, L, R, T are related. Both m and T are directly measurable, but d has to be obtained from o ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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