Wright State University Lake Campus/2016-1/Phy1060/T1 upgrade
So far here are the subpages that have been created. Your's will appear here when you create the page. Use these subpages to document where you have contributed. As you report, refer to the the question number. The first edit by user:Guy vandegriftSock1 was to note that the question mark was missing on problem 4. Template:Subpages/List
Upgrade
1
Stellar parallax is Template:Clear
2
Luminosity is Template:Clear
3
A standard candle isTemplate:Clear
4
Absolute magnitude is Template:Clear
5
Relative magnitude isTemplate:Clear
6
In 1989 the satellite Hipparcos was launched primarily for obtaining parallaxes and proper motions allowing measurements of stellar parallax for stars up to about 500 parsecs away, which is about ____ times the diameter of the Milky Way Galaxy.Template:Clear
7
An object emits thermal (blackbody) radiation with a peak wavelength of 250nm. How does its temperature compare with the Sun? Template:Clear
8
The "normalized intensity" of a Sun-like star situated one parsec from Earth would be 4πI = 1. What is 4πI for a star with 100 times the Sun's energy output that is situated 10pc from Earth?Template:Clear
9
An orbiting satellite makes a circular orbit 5 AU from the Sun. It measures a parallax angle of 0.2 of an arcsecond (each way from the average position). What is the star's distance? Template:Clear
10
A star that is increasing it's temperature while maintaining constant luminosity isTemplate:Clear
11
The range of wavelength for visible light is betweenTemplate:Clear
12
Based on the HR diagrams and images in stars shown in the materials, a very large red supergiant has a diameter that is about ____ greater than a small white dwarf.Template:Clear
13
Why is a star made of plasma? Template:Clear
14
What is the difference between a constellation and an asterism? Template:Clear
15
Stellar parallax is Template:Clear
16
Giant molecular clouds with sufficient conditions to form a star cluster would have formed them long ago. Any stellar births in the past couple of billions years probably resulted from _____ between clouds. Template:Clear
17
A starburst galaxy. Template:Clear
18
Which of the following expresses Jean's criterion for the collapse of a giant molecular cloud of mass, M, radius, R, and temperature T, and pressure P? (Here ? is some constant) Template:Clear
19
Which of the following changes in the properties of a giant molecular cloud might cause it to collapse? Template:Clear
20
What happens if you increase the size of a giant molecular cloud while keeping temperature and mass fixed? Template:Clear
21
What is a Bok globule in the formation of stellar systems? Template:Clear
22
Pre–main sequence stars are often surrounded by a protoplanetary disk and powered mainly by Template:Clear
23
Stars that begin with more than 50 solar masses will typically lose _______ while on the main sequence. Template:Clear
24
The Hayashi and Henyey tracks refer to how T Tauri of different masses will move Template:Clear
25
How do low-mass stars change as they are born?
26
When a star with more than 10 solar masses ceases fuse hydrogen to helium, it Template:Clear
27
Many supernovae begin as a shock wave in the core that was caused by Template:Clear
28
A dying star with more than 1.4 solar masses becomes a ______, and those with more than 5 solar masses becomes a _____ Template:Clear
29
According to Wikipedia, a star with over 20 solar masses converts its Hyrogen to Helium in about 8 billion years, but the conversion of Oxygen to heavier elements take about _____ Template:Clear
30
A grouping with 100 thousand stars would probably be aTemplate:Clear
31
A grouping with a hundred stars is probably aTemplate:Clear
32
I gravity is what holds stars in a cluster together, what is the most important process that causes them to spread apart?Template:Clear
33
Members of an open cluster feel significant forces only due to gravitational interaction with each otherTemplate:Clear
34
Members of an open cluster feel significant forces from nearby giant molecular cloudsTemplate:Clear
35
Members of a globular cluster tend to beTemplate:Clear
36
Members of a globular cluster tend to haveTemplate:Clear
37
In 1917, the astronomer Harlow Shapley was able to estimate the Sun's distance from the galactic centre usingTemplate:Clear
38
Most globular clusters that we see in the sky orbit _____ and have ______ orbitsTemplate:Clear
39
Many stars in a typical open cluster are nearly as old as the universeTemplate:Clear
40
Many stars in a typical globular cluster are nearly as old as the universeTemplate:Clear
41
The number of globular clusters in the Milky way galaxy is aboutTemplate:Clear
42
The location of open clusters can be described asTemplate:Clear
43
Stars can "evaporate" from a cluster. What does this mean?Template:Clear
44
At the center of the Crab nebula is Template:Clear
45
Aside from its location on the HR diagram, evidence that the white dwarf has a small radius can be found fromTemplate:Clear
46
This spectrum of the star Vega suggests thatTemplate:Clear
47
Which of the following is NOT an essential piece of a a strong argument that a white dwarf is not only the size of the earth, but typically has the same mass as the Sun. Template:Clear
48
The course materials presented three arguments suggesting that a white dwarf is roughly the size of the earth. Which best summarizes them?Template:Clear
49
As of 2008, the percent uncertainty in the distance to the Crab nebula is approximately, Template:Clear
50
What was Messier doing when he independently rediscovered the Crab in 1758? Template:Clear
51
What best explains this figure?Template:Clear
52
What causes the blue glow of the Crab nebula?Template:Clear
53
One way to determine the distance to a nebula or small cluster of clouds is to compare the angular expansion to the spectroscopic Doppler shift. Two clusters (A and B) have the same spectroscopically measured velocity. Cluster A is moving towards the observer and exhibits the greater angular expansion. Which cluster is closer? Template:Clear
54
What causes the "finger-like" filamentary structure in the Crab nebula?Template:Clear
55
is the kinetic energy of a solid rotating ball, where M is mass, R is radius, and P is period. And, .
You are banging espressos in a little coffeehouse with your astronomy friends, talking about a new SN remnant that closely resembles the Crab. You have observed the pulsar, and wonder what the total power output of the nebula might be. You know both the period of the pulsar, as well as , which represents the amount of time you think the pulsar will continue pulsing if it continues slowing down at its present rate. What formula do you write on your napkin?Template:Clear
56
In one respect, the universie is arguably "young", considering how much complexity it contains. This is often illustrated by a calculation ofTemplate:Clear
57
Comparing Hubble's original (1929) plot of redshift versus distance with the later one in 2007, the latter extends farther into space by a factor ofTemplate:Clear
58
The course materials present two cosmic expansion plots. Hubble's original (1929) plot usedTemplate:Clear
59
The course materials present two cosmic expansion plots. The more recent (2007) plot usedTemplate:Clear
60
Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distance of 4 cm expands out to 12 cm. To what distance would a raisin originally situated at a distance of 2 cm expand?Template:Clear
61
You at the center raisin of an expanding raisinbread model of Hubble expansion, and from your location a raisin originally situated at a distance of 1 cm expands out to a distance of 4 cm. The nearest raisin with intelligent life is situated exactly halfway between your (central) location and the edge. How would this second "intelligent" raisin view an expansion of a raisin 1 cm away?Template:Clear
62
Place yourself in an expanding raisinbread model of Hubble expansion. A raisin originally situated at a distance of 2 cm expands out to 4 cm. To what distance would a raisin originally situated at a distance of 4 cm expand?Template:Clear
63
This light clock is associated with Template:Clear
64
Suppose the light clock involved a ball being tossed back and forth on a train going just under the speed of sound. In contrast to the situation for light reflecting back and forth on a train going just under the speed of light, there is virtually no time dilation. Why?Template:Clear