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Lecture 1: Observations of planetary systems
Lecture 1: Observations of planetary systems

... Here A is the albedo (typically A = 0.1–0.5). If we assume that A = 0.3 we find that Jupiter reflects fJup = 1 × 10−9 of the Sun’s luminosity, while Earth reflects f⊕ = 2 × 10−10 . We therefore expect planets to be 22–25 magnitudes fainter than their host stars at optical wavelengths. This presents ...
Summary Of the Structure of the Milky Way
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... galactic center and the largest dimension of the Milky Way – the Halo. • In addition, more complex analysis of globular clusters has yielded the orbital speed of the Sun as it orbits the galactic center and the age of the Milky Way. • Finally, when knowledge of the orbital speed of Sun is combined w ...
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... FACT: The damaging UV rays from the sun are reflected from sand, sea, snow, water and other surfaces and so sun damage can occur whilst you are sitting in the shade. Regardless of whether you are in the shade or fully exposed to the sun’s rays, you must take sun protection seriously and use an SPF 3 ...
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... to determine their distances from Earth. Figure 4 shows how a close star’s position appears to change. Knowing the angle that the star’s position changes and the size of Earth’s orbit, astronomers can calculate the distance of the star from Earth. Because space is so vast, a special unit of measure ...
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... Temperature in Celsius or Fahrenheit are conveniences Temperature in Kelvin directly measures how much heat a material has  Temperature in Kelvin is always positive  Nothing actually has a temperature of absolute zero ...
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... e)  This might be true if the visit occurred in the winter when different constellations are visible than in the summer. © 2014 Pearson Education, Inc. ...
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... But there is a snag. The criterion for a dynamically dominant planet depends on two factors: in addition to its mass, its distance from the Sun is also important. The more distant a planetary body is, the greater its mass needs to be for it to dominate its surroundings to the same extent and over th ...
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Stephen Ashworth

... But there is a snag. The criterion for a dynamically dominant planet depends on two factors: in addition to its mass, its distance from the Sun is also important. The more distant a planetary body is, the greater its mass needs to be for it to dominate its surroundings to the same extent and over th ...
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... and 50,000 AU (or some say as great as 200,000 AU) from the Sun and there is indirect evidence for a central doughnut shaped cloud between 2,000 and 20,000 AU called the Hill’s cloud. It must be admitted that there is yet no direct evidence for either the Oort cloud or the Hill’s cloud although indi ...
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... 2. Hold out your fist at an arms distance and carefully rotate your body, keeping your arm stiff, to exactly how many fist-widths fit into the 90 degree angle. a. Example: Say it takes 8 of my fists to cover the 90 degree angle. Then we have: 90/8 = 11 (degrees/fist) 3. Repeat the measurement to see ...
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... gravitational pull of the Sun and the Moon on the Earth's equatorial bulge. Therefore, as it moves through the precessional circle, it moves in little waves with amplitude of 19 arc seconds and a period of 19 years. Proper Motion: This is the rate at which directions in the sky change, in arc second ...
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... are the remains of high-mass stars. They are even smaller and denser than white dwarfs. A neutron star may contain as much as three times the mass of the sun but be only about 25 kilometers in diameter, the size of a city! In 1967, Jocelyn Bell, a British astronomy student, detected an object in spa ...
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... The first class unites the short-lasting prominences. This class is divided into three types: type Ia – loop prominences and coronal rain, type Ib - surge and type Ic – spray prominences. The prominences from the different types have different physical characteristics. For example the surge prominen ...
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... stars and would result in numbers that are cumbersome to use. • B is incorrect because light-years are used to measure distances in the universe and would be too large to use as a measure of the size of stars. • C is correct because the radius of the sun, one solar radius, is used to measure the siz ...
Hipparcos distance estimates of the Ophiuchus and the Lupus cloud
Hipparcos distance estimates of the Ophiuchus and the Lupus cloud

... dark molecular clouds and their dense cores. One of the main motivations for these investigations is the study of the process of star and planet formation in its entirety, and a deeper understanding of the effects of the local environment. A key aspect of the scientific analysis of a dark molecular c ...
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Journey to the Stars Educator`s Guide

... the Big Bang), all that existed in the universe was dark matter and the elements hydrogen, helium, and trace amounts of lithium. Dark matter’s gravity gathered the gas to form the first stars. Over the next few billion years, stars were born more rapidly than at any other period in the history of the ...
Lab 2 - TCNJ
Lab 2 - TCNJ

... path through the sky, with the days growing longer and longer, until it reaches it highest point in the sky on the summer solstice. On the Summer Solstice, which occurs on June 21, the Sun is at its highest path through the sky and the day is the longest. Because the day is so long the Sun does not ...
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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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