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DTU 8e Chap 11 Characterizing Stars
DTU 8e Chap 11 Characterizing Stars

... supergiants, and white dwarfs. The mass-luminosity relation expresses a direct correlation between a main-sequence star’s mass and the total energy it emits. Distances to stars can be determined using their spectral types and luminosity classes. ...
Supermassive black holes
Supermassive black holes

... no obvious spiral arms. Although they can have dust, they have little gas and do not have much star formation and are mostly older stars ...
4 Distances in Astronomy
4 Distances in Astronomy

Orbital Motion and Energy 28. What is the gravitational field strength
Orbital Motion and Energy 28. What is the gravitational field strength

Chapter 9 - Astronomy
Chapter 9 - Astronomy

... wrong. Almost without exception, individual storm cells of upward-moving bright-white clouds exist in the dark-colored bands. This suggests that these bands are the regions of net upward-moving gas motion (the opposite of the standard interpretation). 8. Data from Voyager showed that at the boundari ...
powerpoint - High Energy Physics at Wayne State
powerpoint - High Energy Physics at Wayne State

... The Milky Way Sun is ~ 30000 LY from the center of our Galaxy. From our location within the galaxy, we cannot see through its far rim because the space between stars is not empty – interstellar dust or gas which absorbs visible light. The interstellar gas is the fuel for the formation of stars. Yet ...
The scale of the Universe (along with units and scientific notation)
The scale of the Universe (along with units and scientific notation)

... One of the stars in the Alpha Centauri system, Proxima Centauri, was recently found to have an orbiting planet that might be at just the right temperature to have liquid water… which is promising for the possibility of life ...
Whiteq
Whiteq

... The densities of white dwarves are, of course, very high. Sirius B has a density of about 125,000 g/cm3. The densest may be as much as 10,000 times denser than this. The most dense materials on earth are only about 20 g/cm3. This is why the idea was initially regarded with skepticism. These densitie ...
We Are Made of Stardust
We Are Made of Stardust

... For stars, there is a price to be paid for creativity: The more kinds of atoms created, the shorter-lived the star. Only the chemically laconic are long-lived. The reason pertains to gravity and how gravity determines the extent and pace of nuclear fusion. The more mass (more hydrogen) that a star b ...
L6-Diskproperties
L6-Diskproperties

Lecture 8: The Stars - Department of Physics and Astronomy
Lecture 8: The Stars - Department of Physics and Astronomy

... Pioneers of Stellar Classification A better classification scheme was found by Annie Jump Canon, who joined the “computers” in 1896. Found that stars come in a “natural sequence”. The current scheme of O, B, A, F, G, K, M resulted from Canon revising Fleming’s work. Canon went on to classify 400, ...
Electronic Text Book Unit 11
Electronic Text Book Unit 11

... Dividing the day into equal parts The time of day A clock tells you the exact time of day and is used to mark the division of the day into equal parts. It may be hard to imagine, but there once was a time when humans did not need to keep track of the exact time of day. The rise and fall of the sun w ...
How big are stars? How do we know?
How big are stars? How do we know?

... a) relatively hot main-sequence stars that are relatively close to the Sun. b) relatively cool giant stars that are relatively close to the Sun. c) relatively cool main-sequence stars that are relatively far from the Sun. d) relatively cool main-sequence stars that are relatively close to the Sun. e ...
Orionids meteor shower is in the morning sky and Comet of Century
Orionids meteor shower is in the morning sky and Comet of Century

Constituents of the Milky Way
Constituents of the Milky Way

Science Argumentative Writing Prompt Problem: Scientists have
Science Argumentative Writing Prompt Problem: Scientists have

Galaxies - science9atsouthcarletonhs
Galaxies - science9atsouthcarletonhs

... – Lenticular galaxies are disc galaxies (like spiral galaxies) which have used up or lost most of their interstellar matter and therefore have very little ongoing star formation.[2] As a result, they consist mainly of aging stars (like elliptical galaxies). The dust in most lenticular galaxies is ge ...
9 Dwarf Galaxies
9 Dwarf Galaxies

PH607lec10-4gal2
PH607lec10-4gal2

... up their gas, have older/redder stars)  Late type spirals have substantial on-going star-formation, didn’t form as many stars early-on (and thus lots of gas left) ...
2 Coordinate systems
2 Coordinate systems

... unknown it usually suffices to use two coordinates. On the other hand, since the Earth rotates around it’s own axis as well as around the Sun the positions of stars and planets is continually changing, and the measurment of when an object is in a certain place is as important as deciding where it is ...
HONORS EARTH SCIENCE
HONORS EARTH SCIENCE

... 2. Describe characteristics of Terrestrial planets. 3. Explain the formation of planets in our solar system 4. Explain the cause of a meteor shower 5. Describe what causes a comet’s tail to change 6. Define a planet. Use this to explain why Pluto is not a planet Light, Astronomical Observations and ...
The Milky Way and other Galaxies
The Milky Way and other Galaxies

... Measuring the Mass of the Black Hole in the Center of the Milky Way By following the orbits of individual stars near the center of the Milky Way, the mass of the central black hole could be determined to be ~ 4 million solar masses. ...
Kohoutek Is Coming - Institute of Current World Affairs
Kohoutek Is Coming - Institute of Current World Affairs

... to expect and prepare for another Day of Trouble." But some observers through the ages have seen in comets great beauty and benignity. Here are the concluding words of two scientific lectures on comets delivered in ...
My Favorite Universe
My Favorite Universe

The Science of Life in the Universe
The Science of Life in the Universe

... these stories concerned mythical or supernatural beings, such as gods and others, living among the constellations, but some were not so different from the ideas we consider today. Nevertheless, the present-day search for life in the universe differs from all these ancient speculations in an importan ...
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Rare Earth hypothesis



In planetary astronomy and astrobiology, the Rare Earth Hypothesis argues that the origin of life and the evolution of biological complexity such as sexually reproducing, multicellular organisms on Earth (and, subsequently, human intelligence) required an improbable combination of astrophysical and geological events and circumstances. The hypothesis argues that complex extraterrestrial life is a very improbable phenomenon and likely to be extremely rare. The term ""Rare Earth"" originates from Rare Earth: Why Complex Life Is Uncommon in the Universe (2000), a book by Peter Ward, a geologist and paleontologist, and Donald E. Brownlee, an astronomer and astrobiologist, both faculty members at the University of Washington.An alternative view point was argued by Carl Sagan and Frank Drake, among others. It holds that Earth is a typical rocky planet in a typical planetary system, located in a non-exceptional region of a common barred-spiral galaxy. Given the principle of mediocrity (also called the Copernican principle), it is probable that the universe teems with complex life. Ward and Brownlee argue to the contrary: that planets, planetary systems, and galactic regions that are as friendly to complex life as are the Earth, the Solar System, and our region of the Milky Way are very rare.
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