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Exercise 4 (Stars and the universe) Suggested answers
Exercise 4 (Stars and the universe) Suggested answers

... radiation curve. On the curve, there is a peak which shifts to shorter wavelength when the temperature of the blackbody increases. From the position of the peak, astronomers can deduce the surface temperature of the star. In general, the spectra of hot stars peak at shorter wavelengths and therefore ...
How the universe works – Answer Key Star dust is the building
How the universe works – Answer Key Star dust is the building

BrainPOP - The Science Spot
BrainPOP - The Science Spot

... pulls the clouds together causing clumps to form. If the clump is large enough, the __________ caused by gravity inside a ____________ begins to generate _________. 2. The heat and pressure builds until __________ __________ reactions begin to take place inside the core. Gravity pulls _____________ ...
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell Diagram

Stellar Evolution and the HR Diagram – Study Guide
Stellar Evolution and the HR Diagram – Study Guide

... c. Which is brighter, the sun or a white dwarf? The Sun (but not as hot) d. Is Vega brighter than our sun? Yes (closer to upper top of diagram) e. Is Antares hotter than our sun? No, it’s a giant, class K or M (lower on diagram) 23. Stars that move off the main sequence first move to the _Giant_ reg ...
Inverse Square Law
Inverse Square Law

How it works:
How it works:

... How it works: On the reverse of this sheet are four constellations, all of which can be seen on summer nights in Colorado. Each constellation has five stars. For every book read, fill in one star. Each time you complete a constellation, bring this sheet to the teenseen to receive a prize and a raffl ...
Measuring Distance with Spectroscopic Parallax
Measuring Distance with Spectroscopic Parallax

... 1. Print out the HR diagram. 2. Using a pen or pencil, draw a smooth best-fit curve that runs through the middle of all of your main sequence stars. Just ignore the red giants and white dwarfs for this activity. Note that this will not be a straight line; it will curve slightly. And, it will not go ...
binary stars - El Camino College
binary stars - El Camino College

... Two-thirds of all stars are part of multiple star systems, where two or more stars are born at the same time from the same gas cloud. Only about 30% of all stars are single, like the Sun. The distances between companion stars ranges from less than 10 million miles (0.1 AU), to over 10,000 AU. Simila ...
Chapter 15 (Star Lives)
Chapter 15 (Star Lives)

... D. are at different stages of their lives. 2. In making a model of a star, an astronomer does NOT have to know or assume: A. that the energy given off is produced in the interior. B. the mass of the star. C. the chemical composition of the star. D. the distance to that star. 3. For a star like our s ...
Chap 11 Characterizing Stars v2
Chap 11 Characterizing Stars v2

... A spectroscopic binary is a system detected from the periodic shift of its spectral lines. This shift is caused by the Doppler effect as the orbits of the stars carry them alternately toward and away from Earth. An eclipsing binary is a system whose orbits are viewed nearly edge-on from Earth, so th ...
Slide 1 - Physics @ IUPUI
Slide 1 - Physics @ IUPUI

Nuclear Interactions in Supernovae .
Nuclear Interactions in Supernovae .

AY1 Homework for Quiz 2: Spring 2017
AY1 Homework for Quiz 2: Spring 2017

Star Formation
Star Formation

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Stars and the Main Sequence

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Recap: High Mass Stars

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... Saturn is guaranteed to be the most exciting object in the late spring and early summer sky. It is important to have some interesting stats for the public as they observe this planet. See the last page of the Object Descriptions for relevant facts. We are currently moving apart from our closest poin ...
Types of Stars
Types of Stars

Evolution of Stars and Galaxies
Evolution of Stars and Galaxies

... Prominences: huge, arching gas columns possibly caused by magnetic fields ...
Red Giants - Uplift North Hills Prep
Red Giants - Uplift North Hills Prep

... • done independently by Enjar Hertzsprung and Henry Norris Russell Henry Norris Russell dissuaded Cecilia Payne-Gaposchkin from concluding that the composition of the Sun is different from that of the Earth in her papers, as it contradicted the accepted wisdom at the time. However, he changed his mi ...
AST121 Introduction to Astronomy
AST121 Introduction to Astronomy

Chapter 2: The Sky
Chapter 2: The Sky

... Stars are named by a Greek letter (a, b, g) according to their relative brightness within a given constellation + the possessive form of the name of the constellation: Betelgeuse = a Orionis, Rigel = b Orionis ...
Galaxy Powerpoint
Galaxy Powerpoint

... b.) All that is left is a tiny ball of “lifeless material” ...
Name - MIT
Name - MIT

... A) A 100 kg mass moving at 1 km/s. B) A 20 kg mass moving at 2 km/s. C) A 2 kg mass moving at 5 km/s. D) A 10 kg mass moving at 4 km/s. E) A 5 kg mass moving at 2 km/s. 7) The Homestake Gold Mine experiment was designed to detect neutrinos. What insight can be gained from such an experiment? A) The ...
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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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