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Physics - Content by Unit
Physics - Content by Unit

Week 5 - OSU Astronomy
Week 5 - OSU Astronomy

26.3 Life Cycles of Stars
26.3 Life Cycles of Stars

here
here

Patterns in the Sky
Patterns in the Sky

... of celestial objects. 2. Celestial objects in the Solar System have unique properties. 3. Some celestial objects can be seen with the unaided eye and can be identified by their motion. 4. The Sun emits light and other forms of radiant energy that are necessary for life to exist on Earth. 5. Satellit ...
Word - Sam Davyson
Word - Sam Davyson

... R observed This result makes sense as if  = 0 then the ratio of the distances is 1, implying that they are the same. And also if  > 0 then the answer will always be greater than 1 suggesting a greater observed than emitted distance. Once again the  is determined from the movement of the black ...
Stars
Stars

... ice starts to melt. This lets the dust and gas out.  Solar winds then push them away from the comet. This makes the comet's tail.  Every time a comet comes close to the Sun, a part of it melts. Over time, it will completely ...
Astronomy
Astronomy

... • The center of the galaxy is about 25,000 lightyears away, but it is hidden from view by large clouds of dust and gas. • The Milky Way might contain 1 trillion stars. • It takes the Sun 225 million years to orbit the center of the Milky Way. • Like many other galaxies, the Milky Way has a supermass ...
The Universe
The Universe

... Black holes are the strangest objects in the Universe. A black hole does not have a surface, like a planet or star. Instead, it is a region of space where matter has collapsed in on itself. This catastrophic collapse results in a huge amount of mass being concentrated in an incredibly small area. Th ...
Lect12-3-10-10
Lect12-3-10-10

... stars. Their radiation is energetic enough to ionize the surrounding gas and heat it up, so that the gas that did not collapse into these young stars is pushed away. Behind the visible nebula is a dense cloud of molecular hydrogen gas, from which infrared observations show that many more stars have ...
Stellar Classification
Stellar Classification

Document
Document

... • As the helium core grows, it compresses. Helium doesn’t fuse to heavier elements for two reasons. (1) with 2 p+ per nucleus, the electric repulsion force is higher than was the case for H-fusion. This means that helium fusion requires a higher temperature than hydrogen fusion -- 100 million K (2) ...
Hinsdale Astro TEST
Hinsdale Astro TEST

... b. The first generation stars formed such a long time ago that the light from them has not yet had time to reach us. c. The first generation stars were all very massive and exploded as supernova. d. The first generation stars formed with only H and He and therefore have no spectral features. e. We d ...
Section C - Astrophysics
Section C - Astrophysics

... merely used as a catalyst. Even heavier elements (up to iron) can be produced in nuclear fusion at yet higher temperatures in higher mass stars, viz. Carbon burning (C producing O, Ne) at 5 × 108K (M> 8M) Neon burning (Ne producing O, Mg) at 1.5 × 109K (M > 5M) Oxygen burning (producing elements u ...
How many planets are there in the galaxy?
How many planets are there in the galaxy?

Matariki-Maori New Year
Matariki-Maori New Year

... away (our Sun is 8 light minutes away) • The blue color is caused by blue light being scattered by dust. • The stars in the Pleiades are young100 million years old about 1/50th the age of our Sun ...
Document
Document

... What proof is there of black holes? What proof is there that black holes are black? Why should light be affected by gravity? What proof is there that it is? ...
Review Sheet and Study Hints - Tufts Institute of Cosmology
Review Sheet and Study Hints - Tufts Institute of Cosmology

...  Difference between GTR and Newtonian Gravity  Principle of Equivalence  Proof of GTR  Understand Einstein’s “Link” between Structure of Space time and Kinematics  The Cosmological Principle  What does it state?  What’s the meaning of Homogeneous and Isotropic  Is the Universe truly homogene ...
Chapter 15 part 1
Chapter 15 part 1

... 1. Hotter objects emit more light per unit area at all frequencies. (Brighter) 2. Hotter objects emit photons with a higher average energy. (Bluer) ...
No Slide Title
No Slide Title

... The Sun is the nearest star to Earth. The sun is just an ordinary star. The next brightest star to us is called Alpha Centauri. Light from Alpha Centauri takes 4.3 years to get to us. Light from our sun only takes 8 minutes. Alpha Centauri are really three stars all orbiting each other. One of thes ...
2. - Quia
2. - Quia

... spacecraft is actually headed towards Sirius. If there is an intelligent civilization living on a planet near that star, how many years will it be until Voyager reaches it? 3. Do you think that it is possible that one of the Voyager spacecraft would ever be intercepted by a civilization around anoth ...
Chapter21
Chapter21

... 15. If the mass-losing star is more massive, the separation of the two stars decreases, and the mass-losing star continues to fill its Roche lobe even as it loses mass. 16. They lose orbital energy through friction with gas in the common envelope. 17. The two stars can exceed escape velocity and go ...
Today`s Powerpoint - Physics and Astronomy
Today`s Powerpoint - Physics and Astronomy

... random directions. Photons of other wavelengths go through. Get dark absorption line at green part of spectrum. ...
Microsoft Power Point version
Microsoft Power Point version

... Spectral type is determined by a star’s surface temperature. ...
Can you write numbers in scientific notation
Can you write numbers in scientific notation

... Do you understand the importance of studying binary star systems? Are you able to describe the different ways binary stars are observed? You should be able to identify what factors would prevent us from observing a binary star system in particular way (e.g. why might we not see a binary system as a ...
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Star formation



Star formation is the process by which dense regions within molecular clouds in interstellar space, sometimes referred to as ""stellar nurseries"" or ""star-forming regions"", collapse to form stars. As a branch of astronomy, star formation includes the study of the interstellar medium (ISM) and giant molecular clouds (GMC) as precursors to the star formation process, and the study of protostars and young stellar objects as its immediate products. It is closely related to planet formation, another branch of astronomy. Star formation theory, as well as accounting for the formation of a single star, must also account for the statistics of binary stars and the initial mass function.In June 2015, astronomers reported evidence for Population III stars in the Cosmos Redshift 7 galaxy at z = 6.60. Such stars are likely to have existed in the very early universe (i.e., at high redshift), and may have started the production of chemical elements heavier than hydrogen that are needed for the later formation of planets and life as we know it.
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