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What is a white dwarf?
What is a white dwarf?

... Shrinkage of White Dwarfs • Quantum mechanics says that electrons in the same place cannot be in the same state • Adding mass to a white dwarf increases its gravity, forcing electrons into a smaller space • In order to avoid being in the same state in the same place some of the electrons need to mo ...
Opakování z minulého cvičení
Opakování z minulého cvičení

... Josef von Fraunhofer (1787-1826) in 1814. He was the first person to study the rainbow pattern produced by passing light through a prism in detail under intense magnification. He was actually interested in the properties of the glass in the prisms, and how in affected the light, but to his surprise ...
File
File

pluto: a human comedy
pluto: a human comedy

... thin disc of material, so that the 8 planets and the numerous asteroids orbit the Sun very nearly in the same plane. Pluto, on the other hand, has an orbital plane which is inclined at an angle of about 16° with respect to this plane. 3. Before the discovery of Pluto, the 8 planets could be divided ...
The astronauts in the upper left of this photo are working on the
The astronauts in the upper left of this photo are working on the

... Astronauts who spend long periods in outer space could be adversely affected by weightlessness. One way to simulate gravity is to shape the spaceship like a cylindrical shell that rotates, with the astronauts walking on the inside surface (Fig. 5–32). Explain how this simulates gravity. Consider (a) ...
How Big is the Universe
How Big is the Universe

... understand. Scientists and astronomers sometimes use a light-year, the distance light travels in one year, to measure these distances. Earth is about 93,000,000 miles away from the Sun. It takes light from the Sun 8.3 minutes to reach the Earth. We use the speed of light to measure the time it takes ...
Building` a Galaxy SED
Building` a Galaxy SED

... cosmology, large variation in physics (fluid dynamics, quantum physics) Practical problem: galaxies are biased tracers of underlying mass distribution. In order to use galaxies to measure underlying mass distribution, we must understand galaxies. ...
astronomy
astronomy

... countless stars and wondered at the incredible sights there. One thing is clear, however: the basic practice of astronomy had been well established by the time humans formed the first civilisations. Since the beginning of human history, people from nearly every culture have gazed into the sky and in ...
Document
Document

... even those which are predominantly Catholic such as Italy, you see very low birth rates,” Professor Bennet says, “Yet in the developing world they’re off the scale. The data suggests that if you take a dollar spent on enforcing child limitation policies and instead spend it on education and opportun ...
The Earth--Our Observing Platform
The Earth--Our Observing Platform

... Purpose: To provide activities to help one better appreciate what we see from the Earth as we look toward the sky, and realize modern physical science was born from efforts to make sense of those observations. These activities will both help you "see the big picture" and reinforce specific concepts ...
Day 3
Day 3

... We highlight the importance of gaseous TiO and VO opacity on the highly irradiated close-in giant planets. The dayside atmospheres of these planets naturally fall into two classes that are somewhat analogous to the M- and L-type dwarfs. Those that are warm enough to have appreciable opacity due to T ...
Chapter 17 Star Stuff
Chapter 17 Star Stuff

Chapter 17 Star Stuff How does a star`s mass affect nuclear fusion
Chapter 17 Star Stuff How does a star`s mass affect nuclear fusion

Geosystems-7th-Edition-Christopherson-Solution
Geosystems-7th-Edition-Christopherson-Solution

... size, and relationship to its planets. Our Sun is both unique to us and commonplace in our galaxy. It is only average in temperature, size, and color when compared with other stars, yet it is the ultimate energy source for almost all life processes in our biosphere. Planets do not produce their own ...
Earth Science 24.3 The Sun
Earth Science 24.3 The Sun

... eat, has somehow come from solar energy. The sun is also important to astronomers, since until recently, it was the only star we could study the surface of. Even with the largest telescopes, most other stars appear only as points of light. ...
The Changing Earth Atmosphere
The Changing Earth Atmosphere

... A. The Current Earth’s Atmosphere 1. Composition of the Atmosphere. a) The Earth’s atmosphere is simply called air. It is primarily composed of many discrete gases, each with its own physical properties, in which varying quantities of tiny solid and liquid particles are suspended. b) ...
LESSON 8: STARS
LESSON 8: STARS

... While the thousands of stars in the night sky appear to be very similar, they are more distinct from one another than their appearance would suggest. Stars have various sizes, masses, temperatures, colours, luminosities, compositions and lifecycles. The largest stars are several hundred times the d ...
Stellar Physics 1
Stellar Physics 1

... A. The track that a star takes as it moves up the main sequence. B. The track that a star takes as it moves down the main sequence. C. The track that a star takes as it moves off the main sequence. y D. The track that a star takes as it moves onto the main sequence. ...
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p - INAF-OAT Trieste Users site

... relatively fast evolution of the stellar luminosity, which limits the continuous habitability (required for life to evolve into complex forms) ...
Doppler Effect
Doppler Effect

... or both move Approach  Shift to shorter λ  Blue shift (moving toward) higher f Recede  Shift to longer λ  Red shift (moving away) lower f Bigger shift (change) in λ  Bigger speed ...
Santos: On the relation between stars and their planets
Santos: On the relation between stars and their planets

ppt
ppt

... Hubble could only find Cepheids in the closest few galaxies (1-2 Mpc). Even Hubble Space Telescope cannot find Cepheids beyond the Virgo cluster (16 Mpc). Beyond 1-2Mpc, Hubble used… ...
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... different stars can be seen in different seasons. B. Students know the way in which the Moon’s appearance changes during the four-week lunar cycle. C. Students know telescopes magnify the appearance of some distant objects in the sky, including the Moon and the planets. The number of stars that can ...
Seeing Through the Clouds of Venus
Seeing Through the Clouds of Venus

... •  The sun gets ~6% more luminous every 1 billion years •  As the sun gets brighter (hotter) with time, the region around the star where habitable planetary temperatures are possible gets pushed outward At  a  later  Sme:   Sun  is   brighter   ...
Lecture 10 - Lick Observatory
Lecture 10 - Lick Observatory

... from Kepler’s law, semi-major axis: 2 AU A:conservation semi-major axis = 2 AUmomentum and conservation of energy of angular ...
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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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