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HR Diagram Lab Handout
HR Diagram Lab Handout

... 7. The temperature of the hottest stars is _______________. 8. The color of the hottest stars is ________________. 9. The temperature of the coldest stars is _______________. 10. The color of the coldest stars is ________________. 11. The life expectancy of a very hot star is _______________ years. ...
RR animation
RR animation

... • Stars that exhibit pulsation periods on the order of a few days to months, are 4–20 times more massive than the Sun, and up to 100,000 times more luminous. • Cepheids are supergiants of spectral class F6 – K2 and their radii change by several million km (30%) in the process. • There exists a well- ...
(as Main Sequence Stars)?
(as Main Sequence Stars)?

... temperature from spectrum (black-body curve or spectral lines), then find surface area, then find radius (sphere surface area is 4 p R2) ...
star life cycle
star life cycle

... It will use up most of its hydrogen (this makes it lighter so there is not enough gravity to keep the gases together) ...
Russell County Schools Non-Traditional Instructional Expectations
Russell County Schools Non-Traditional Instructional Expectations

Supernovae – the biggest bangs since the Big Bang
Supernovae – the biggest bangs since the Big Bang

... Sun, it will make a huge explosion.  The entire white dwarf will explode with the energy of four billion Suns.  This is called a “white dwarf supernova” (also known as a “Type Ia supernova”). Imagine you made a series of bombs, each with the same amount of the same material.  The bombs would all hav ...
Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

... • Cataclysmic or explosive variable stars: – Stars that irregularly increase in brightness by a large factor. – Nova or dwarf nova: occurs in semidetached binaries where a white dwarf star is accreting matter from an ordinary companion star. When the accreted layer is about half a meter thick, the t ...
Stellar Classification and Evolution What is a star? A cloud of gas
Stellar Classification and Evolution What is a star? A cloud of gas

... from helium fusion _____________ much of their mass  The ejected material expands and cools, becoming a planetary ________________ (which actually has nothing to do with planets, but we didn’t know that in the 18th century when Herschel coined the term)  The core _____________________ to form a Wh ...
1. Base your answer to the following question
1. Base your answer to the following question

... (3) ultraviolet-ray end of the electromagnetic spectrum (4) gamma-ray end of the electromagnetic spectrum 27. The diagram below shows a standard spectrum compared to a spectrum produced from a distant star. ...
PHY2083
PHY2083

... i) Msun = msun - 5 lg (d) + 5 d = 1 AU = 4.848 x 10-6 pc => Msun = -26.83 - 5 lg (4.848 x 10-6) + 5 => Msun = +4.74 ii) F = L / 4πr2 c.f. previous example at 1 AU now 10 pc = 2.063 x 106 AU Inverse square law => flux will be 1 / (2.063 x 106)2 times lower => Flux at 10pc = 3.21 x 10-10 W / m2 ...
Chapter 21 notes - Clinton Public Schools
Chapter 21 notes - Clinton Public Schools

... Section 5: The Expanding Universe: How the universe was formed: Astronomers believe the universe was incredibly hot and dense, exploded in what astronomers called the Big Bang. According to the big bang theory, the universe formed in an instant, billion of years ago, in an enormous explosion. Since ...
17Nov_2014
17Nov_2014

... • As a red giant expands, it cools – Outer layers cool enough for carbon flakes to form – Flakes are pushed outward by radiation pressure – Flakes drag stellar gas outward with them ...
Suns .n. Stars
Suns .n. Stars

... from Earth. • The sun rises in the east every morning. • The sun gives us light and heat. • The sun has a core in the centre of it. • The sun is about 5,000 degrees but the core is 3 times as hot. • It takes light about 8 minutes 70 seconds to get from Sun to Earth. ...
Astrophysics E1. This question is about stars.
Astrophysics E1. This question is about stars.

... Option E — Astrophysics E1. This question is about the relative population density of stars and galaxies. The number of stars around the Sun, within a distance of 17 ly, is 75. The number of galaxies in the local group, within a distance of 4.0 x 106 ly from the Sun, is 26. (a) Calculate the average ...
Take Home #2 Complete the following on your own paper. Do not
Take Home #2 Complete the following on your own paper. Do not

... A. As more massive stars are examined, temperature and pressure are seen to be greater, and heavier elements are produced B. As more massive stars are examined, temperature and pressure are seen to be less, and lighter elements are produced C. As less massive stars are examined, temperature and pres ...
Jeopardy - Cloudfront.net
Jeopardy - Cloudfront.net

... a. absorption spectrum of elements to the emission spectra of a star b. continuous spectrum of elements to the emission spectra of a star c. emission spectrum of elements to the absorption spectra of a star d. emission spectrum of elements to continuous spectra of a star ...
Ch 19 Directed Reading
Ch 19 Directed Reading

... 13. top of modern H-R diagram 14. bottom of modern H-R diagram 15. right side of modern H-R diagram 16. left side of modern H-R diagram ...
Name ______KEY Date Core ______ Study Guide Galaxies and the
Name ______KEY Date Core ______ Study Guide Galaxies and the

... When did the Big Bang happen and what has happened since? The big bang theory is theorized to have happened 14 billion years ago when the universe suddenly began to expand from one merged mass of matter or substance. At that time, all matter was dense and hot and the universe developed in less than ...
Outline 8: History of the Universe and Solar System
Outline 8: History of the Universe and Solar System

... Total time is 5 hours. Total distance is 380 miles. If you were observed traveling at 60 mph and had covered 380 miles, the assumption would be made that you had traveled for 6 hours and 20 minutes (380miles/60mph) rather than 5 hours. ...
STEM for TY Teachers
STEM for TY Teachers

... 200,000 times more massive). They will eventually lose their heat and become a cold, dark black dwarf. Our Sun will someday turn into a white dwarf and then ultimately a black dwarf. The companion of Sirius is a white dwarf. ...
The life of Stars
The life of Stars

... • Radius: 10-100 solar radii ...
Binary Star - Armagh Observatory
Binary Star - Armagh Observatory

... 200,000 times more massive). They will eventually lose their heat and become a cold, dark black dwarf. Our Sun will someday turn into a white dwarf and then ultimately a black dwarf. The companion of Sirius is a white dwarf. ...
Star Formation
Star Formation

... they strike matter • Very massive stars are so luminous that the collective pressure of photons drives their matter ...
test - Scioly.org
test - Scioly.org

... white dwarfs? What is the surface temperature of that dwarf? 10. What is the spectral type of Mira A? 11. Out of the Science Olympiad 2017 DSO list, which DSO was observed in 1572? 12. Out of the Science Olympiad 2017 DSO list, which DSO is in the Pinwheel Galaxy? 13. Out of the Science Olympiad 201 ...
using a cepheid variable to determine distance
using a cepheid variable to determine distance

... 4. Distance modulus ( m - M ) = _________ 5. Distance to the Cepheid ( r ) = _______ parsecs Distance to the Cepheid ( r ) = _______light years ...
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Perseus (constellation)



Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.
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