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lect3 — 1 Measuring stars: What can be measured?
lect3 — 1 Measuring stars: What can be measured?

... Vega is now known to be a slightly variable star!). For optical bands, Johnson and AB magnitudes are (by construction) similar. But for other bands e.g. infrared or ultraviolet, they can be quite different. So when someone quotes you a magnitude, it pays to ask which system! Absolute magnitude: In a ...
Siriusposter
Siriusposter

Basic properties of stars
Basic properties of stars

... star cluster can tell us how old it is. This is data for NGC 2482. It is about 400 million years old. Stars considerably right of the main sequence are more distant giants. ...
Section 27.2
Section 27.2

Lecture 17 Review
Lecture 17 Review

w 2012-01-13 Stellar Life Cycle
w 2012-01-13 Stellar Life Cycle

reach for the stars
reach for the stars

HW11
HW11

... difficult to apply these concepts to the material for this exam. Review your last exam and be sure that you understand why certain answers are correct, and others are wrong. New material for this Exam ...
Photometry
Photometry

... than the larger magnitudes. As you move up the y-axis, therefore, the numbers will get smaller. We’ll come back to the HR diagram later. Absolute magnitude (M) is a measure of how bright a star actually is. Again, the lower the magnitude, the brighter the star. (The drawn-out definition of absolute ...
Page 1 of 4 KEY PSCI 1055 Test #4 (Form A) KEY Spring 2008
Page 1 of 4 KEY PSCI 1055 Test #4 (Form A) KEY Spring 2008

1 Sep: 6.13am BST 15 Sep: 6.43am BST 30 Sep: 7.14am BST
1 Sep: 6.13am BST 15 Sep: 6.43am BST 30 Sep: 7.14am BST

... and Aquila (the Eagle) whose brightest stars of Deneb, Vega and Altair respectively make up the Summer Triangle. The Swan’s beak is marked by Albireo and halfway between Albireo and Altair is Sagitta (the Arrow) a small but lovely constellation representing an arrow sailing harmlessly between the tw ...
The Stars: Distance, Luminosity, Size
The Stars: Distance, Luminosity, Size

... The idea is that a large sample of stars will contain examples of all life stages (newborn, adult, moribund) and of all types of stars. The hope is that by looking at some carefully selected observable properties of the stars, we will see trends that are the telltale of stellar evolution A large sam ...
Problem Set No. 5
Problem Set No. 5

... 2. Why do some astronomers say that brown dwarfs are not really stars? Why are brown dwarfs hard to study? Some astronomers would say that true stars must have nuclear fusion as an internal energy source. Brown dwarfs are too cool the burn hydrogen. Even though there are nearby brown dwarfs, their ...
Chapter 12 Stellar Evolution
Chapter 12 Stellar Evolution

... Which of the following are old stars with no current nuclear reactions? A. red giants B. main sequence stars C. white dwarfs D. proto stars ...
Apparent Magnitude - RanelaghALevelPhysics
Apparent Magnitude - RanelaghALevelPhysics

... emitted per second (units of Watts). • The Sun’s luminosity is about 4 x 1026 W. • The most luminous stars have a luminosity of about million times that of the Sun! ...
Constellations - Brown University Wiki
Constellations - Brown University Wiki

Chapter 20 Stellar Evolution (20.1-20.3)
Chapter 20 Stellar Evolution (20.1-20.3)

... large numbers of stars, we are looking at stars borne at different times in the 10Gyr history of our Galaxy, so they are in different phases of evolution. Observation of stars in star clusters help, by giving us a look at stars that were all born at the same time. However we use the observations, ou ...
15-1 Notes - westscidept
15-1 Notes - westscidept

... use a ________________ to separate a star’s light into a spectrum. The spectrum gives information about the ______________ and temperature of a star. When a chemical element emits ________, only some colors in the spectrum appear. These are called ____________ lines. The __________ atmosphere of a s ...
Problem Set 2
Problem Set 2

proper motion
proper motion

monkeyball_lifecycleofastar
monkeyball_lifecycleofastar

9. Lectures on Star Formation.
9. Lectures on Star Formation.

Star and Galaxies Chapter 13
Star and Galaxies Chapter 13

... • Middle aged, absolute magnitude is about average • Shines yellow light • Takes 8 minutes for light to reach earth • It is unusual in fact it is found as a single star (normally stars are in groups of 2 (binary system) • Star clusters: group of stars that have a gravitation attraction to each other ...
Powerpoint
Powerpoint

... determine temperature from spectrum (black-body curve or spectral lines), then find surface area, Surface area  Luminosity / (temperature) 4 then find radius (sphere surface area is 4 R2) ...
Hungry Young Stars: A New Explanation for the FU Ori Outbursts
Hungry Young Stars: A New Explanation for the FU Ori Outbursts

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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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