Pulsars - Study guides, Class notes & Summaries
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ASTR 114 Astronomy - Final Exam "Cheat Sheet" | Latest 2023-2024
- Exam (elaborations) • 6 pages • 2023
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-1.5 magnitude Sirius appears 25x brighter 
than 2 magnitude Polaris. 
 “All neutron stars are pulsars, but not all 
pulsars are neutron stars” FALSE 
 “Spectroscopic Binary” is the term given to 
a pair of stars that we can determine are 
orbiting each other only by measuring their 
periodic Doppler shifts. 
 A 6.8 solar mass neutron star does NOT 
exist. 
 A loop of gas and charged particles 
following the magnetic field lines between 
sunspot’s poles is a Prominence/...
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ASTRO 205 (Quasars, Black Holes and Pulsars) Midterm 1 Test Questions and Answers
- Exam (elaborations) • 21 pages • 2024
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ASTRO 205 (Quasars, Black Holes 
and Pulsars) Midterm 1 Test 
Questions and Answers
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AST 111 Final Exam || A+ Graded Already.
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White Dwarf "Star" correct answers Result of the death of a low mass star 
 
The exposed core of a low mass star; 
-hot 
-dense 
-mostly carbon 
 
If there is no new energy production in a white dwarf, what prevents gravity from crushing it? correct answers Electron degeneracy pressure 
 
White dwarf "stars"- electron degeneracy pressure correct answers Electron degeneracy pressure will only hold up a star to about 1.4 solar masses, above that gravity will begin to win, resulting in the st...
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ASTR 1020 Final Exam Study Guide 2024
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White dwarfs: properties - Remaining cores of dead, low mass stars 
Electron degeneracy pressure supports them against gravity 
Slowly fade with time 
Sirius and its hot WD companion 
White dwarfs with same mass as Sun are about same size as Earth; slowly cooling 
Typical density 10^6 gram / cubic cm 
Higher mass white dwarfs are smaller 
Cannot be more massive than 1.4MSun, the Chandrasekhar limit 
 
WDs in binaries: nova, supernova Type I - Mass falls toward white dwarf from binary companion 
...
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PSU ASTRO 1 Exam 3 Study Guide | Questions with 100% Correct Answers | Verified | Latest Update 2024
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Explain how a white dwarf's observable properties (specifically Luminosity & Temp) change over billions 
of years if it is left alone, and show how its location would change on an H-R diagram. - •White 
Dwarfs are low-mass stars, and if they are left alone, they will fade and cool forever. 
•If mass transfer adds mass to a White Dwarf, it can become, (1) a Nova, or (2) a Supernova 
Compared to a white dwarf, a neutron star's density is? - •Not all neutron stars are called pulsars 
becaus...
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PHYS 1031A Final Exam Review questions and answers
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What observational measurement is required to determine the distance to a 
Galaxy using Hubble's Law? - ANSWER-Redshift 
What were the conditions of the early universe? - ANSWER-Hot and very dense 
True or False: 
If Light traveled for 5 billion years, then the distance between the two galaxies 
must have been less than 5 billion light years when the light began its journey 
because the distances between galaxies are always increasing in the expanding 
universe - ANSWER-True 
If our universe is...
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PHYS 1031A Final Exam Review questions and answers
- Exam (elaborations) • 5 pages • 2024
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What observational measurement is required to determine the distance to a 
Galaxy using Hubble's Law? - ANSWER-Redshift 
What were the conditions of the early universe? - ANSWER-Hot and very dense 
True or False: 
If Light traveled for 5 billion years, then the distance between the two galaxies 
must have been less than 5 billion light years when the light began its journey 
because the distances between galaxies are always increasing in the expanding 
universe - ANSWER-True 
If our universe is...
-
PHYS 1031A Final Exam Review questions with complete solution
- Exam (elaborations) • 5 pages • 2024
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What observational measurement is required to determine the distance to a 
Galaxy using Hubble's Law? - ANSWER-Redshift 
What were the conditions of the early universe? - ANSWER-Hot and very dense 
True or False: 
If Light traveled for 5 billion years, then the distance between the two galaxies 
must have been less than 5 billion light years when the light began its journey 
because the distances between galaxies are always increasing in the expanding 
universe - ANSWER-True 
If our universe is...
-
PSU ASTRO 1 Exam 3 Study Guide | Questions with 100% Correct Answers | Verified | Latest Update 2024
- Exam (elaborations) • 5 pages • 2023
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Explain how a white dwarf's observable properties (specifically Luminosity & Temp) change over billions 
of years if it is left alone, and show how its location would change on an H-R diagram. - •White 
Dwarfs are low-mass stars, and if they are left alone, they will fade and cool forever. 
•If mass transfer adds mass to a White Dwarf, it can become, (1) a Nova, or (2) a Supernova 
Compared to a white dwarf, a neutron star's density is? - •Not all neutron stars are called pulsars 
becaus...
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ASTR 50 Exam 3 Questions And Answers
- Exam (elaborations) • 5 pages • 2024
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A graduate assistant in astronomy needs to measure the mass of a spiral galaxy. Which of the following observations would be important for her to make? - ️️Obtain the speed at which stars or gas near the outer regions of the galaxy are moving around 
A star whose temperature is increasing but whose luminosity is roughly constant moves in what direction on the H-R diagram - ️️Left 
A type of star cluster that contains mostly very old stars is - ️️a globular star cluster 
A white dwarf...
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