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The Origin of Stars
The Origin of Stars

... object with an accretion disk and jets 4) When the young stellar object begins fusing hydrogen into helium it becomes a true star ...
Scientists classify stars by
Scientists classify stars by

... 2. If the remaining mass of the star is about 1.4 times that of our Sun, it will collapse further to become a neutron star. 3. If the remaining mass of the star is more than about three times that of the Sun, it will collapse and what is left behind is an intense region of gravity called a black hol ...
Handout 15: Virial Theorem E = P.E. + K.E = (1/2)P.E. = -K.E.
Handout 15: Virial Theorem E = P.E. + K.E = (1/2)P.E. = -K.E.

... For a star, gas is compressible, therefore density increases as r decreases Therefore more tightly bound than constant density Therefore PE is more negative than this ...
Measuring the Distance to Stars Using Parallax
Measuring the Distance to Stars Using Parallax

Startalk
Startalk

How Is a Star`s Color Related to Its Temperature? - d
How Is a Star`s Color Related to Its Temperature? - d

... On a clear night you have surely noticed that some stars are brighter than others. But stars also have different colors. Rigel is blue, and Betelgeuse is red. Capella and our sun are yellow. In this activity you will make your own HertzsprungRussell diagram. You will see how star brightness, color, ...
Quiz 1 Review
Quiz 1 Review

... Neutron stars spin extremely fast (1000 times per second). Any remaining electrons not fused with protons are excited by the stars rotation and interact with the neutron stars magnetic field. This interaction releases huge amounts of energy from the neutron stars N and S pole and they are seen as pu ...
Astrophysics
Astrophysics

... but continues to do so until it becomes nothing more than a point mass. Point mass  singularity, and this breaks the laws of Physics. The strength of gravity inside a black hole is so massive that nothing can escape, not even light (which is why they are not visible). The perimeter at which light c ...
S1E4 Extreme Stars
S1E4 Extreme Stars

... What is a planetary nebula? (1) A large swarm of planets surrounding a star. (2) A disk of gas and dust around a young star. (3) Glowing gas in Earth’s upper atmosphere. (4) Ionized gas around a white dwarf star. ...
The portion of light we detect from a star/blackbody depends on
The portion of light we detect from a star/blackbody depends on

stars
stars

Astronomical distances and Stellar magnitudes
Astronomical distances and Stellar magnitudes

... 1. What is meant by a light year? 2. What is meant by an astronomical unit (AU)? 3. What is meant by a parsec (pc)? 4. What is meant by a mega parsec (Mpc)? 5. What is meant by the apparent magnitude of an astronomical object? 6. Give the approximate distance of the following in AU: (a) Sun to the E ...
Chandra Sees the Atmosphere of a Neutron Star - Chandra X
Chandra Sees the Atmosphere of a Neutron Star - Chandra X

... the central region of the supernova remnant Cassiopeia A. This interstellar cloud 14 light years across, is all that remains of a massive star that exploded 330 years ago. A careful analysis of the X-ray data has revealed that the dense neutron star left behind by the supernova has a thin carbon atm ...
File
File

... million K, the surface would be liquid form, while if it's cooler than that, it would be solid. Below that is a solid crust, about a kilometer thick. This crust is very hard and very smooth. Gravity would probably prevent any irregularities larger than half a centimeter. ...
Test 1 - Brock physics
Test 1 - Brock physics

chap17_s05_probs
chap17_s05_probs

... temperature relation for stars. Given two of these values, the third value is found using this relation, described on page 449 in the text. In solar units, L = R2 x T4 , substituting into the expression gives 64 = R2 x 24 , 64 = R2 x 16 Dividing each side of the expression by 16 gives, R2 = 4, there ...
Lec11_2D
Lec11_2D

... Accretion Disks and Black Holes The accretion disk around a black hole can extend very close to the event horizon. The gas speed there is very close to the speed of light, so the friction in the disk is extremely intense. This type of disk will produce the most-energetic x-rays. ...
RED GIANTS
RED GIANTS

... • The H-R Diagram makes a useful roadmap for following stellar evolution. ...
Brock physics - Brock University
Brock physics - Brock University

chap17_f04_probs
chap17_f04_probs

... relation for stars. Given two of these values, the third is found using that relation, described on pg 449 in the text. In solar units, L = R2 x T4 , substituting into the expression gives 64 = R2 x 24 , 64 = R2 x 16 Dividing each side of the expression by 16 gives, R2 = 4, therefore R = 2. The star ...
Name: Period: Date: The Celestial Sphere What is the Celestial
Name: Period: Date: The Celestial Sphere What is the Celestial

... The “road of the sun” on the Celestial Sphere 1. The sun has a _________________ (daily) motion from east to west due to the earth’s spinning around its axis, ~ 24 h 2. The sun also changes its ____________________ in the sky ~ 1 degree per day, ~ 365.25 days What is the ecliptic? ...
10 relativity, black holes_
10 relativity, black holes_

... Depends on the gravity between you and the object you want to escape! For a black hole, the escape velocity (inside the event horizon) is greater than the speed of light! ...
Stars
Stars

... • Then, star collapses under the weight and because it is electron degenerate, energy created will not expand the star and shut off the fusion. • So, entire star (carbon, mostly) undergoes fusion at once. What a star normally takes billions of years to burn, this star burns all at once. BIG explosio ...
Measuring the Stars
Measuring the Stars

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Dyson sphere

A Dyson sphere is a hypothetical megastructure that completely encompasses a star and hence captures most or all of its power output. It was first described by Olaf Stapledon in his science fiction novel, ""Star Maker"". The concept was later popularly adopted by Freeman Dyson. Dyson speculated that such structures would be the logical consequence of the long-term survival and escalating energy needs of a technological civilization, and proposed that searching for evidence of the existence of such structures might lead to the detection of advanced intelligent extraterrestrial life. Different types of Dyson spheres correlate with information on the Kardashev scale.Since then, other variant designs involving building an artificial structure or series of structures to encompass a star have been proposed in exploratory engineering or described in science fiction under the name ""Dyson sphere"". These later proposals have not been limited to solar-power stations. Many involve habitation or industrial elements. Most fictional depictions describe a solid shell of matter enclosing a star, which is considered the least plausible variant of the idea (see below). In May 2013, at the Starship Century Symposium in San Diego, Dyson repeated his comments that he wished the concept had not been named after him.
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