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File - Mr. Gray`s Class
File - Mr. Gray`s Class

... day, it would trace out a Diurnal Circle. – This the circular path a star appears to take each day.  We can’t see stars during the daytime because of the sun, so we don’t actually see the circle. ...
Kepler`s Laws, Newton`s Laws, and the Search for New Planets
Kepler`s Laws, Newton`s Laws, and the Search for New Planets

... Laws: the discovery of extrasolar planets during the past decade, none of which has been observed directly, but whose existence and orbital parameters have been deduced by detecting and analyzing the motion of the stars that they orbit. Two other considerations make the correct way of treating the s ...
Astrophysics - Student Reference Packet
Astrophysics - Student Reference Packet

... stays in the same place and the other stars appear to move in circular paths around this “celestial pole”. They complete one rotation every 24 hrs (called diurnal motion) although we can only observe part of their path (we can’t see them during the day because the scattered blue light of our Sun is ...
Is there life in space? Activity 4: Habitable Conditions
Is there life in space? Activity 4: Habitable Conditions

... A. Student answers will vary. Q. Explain what influenced your certainty rating in the last question. A. Student answers will vary. Answers may include a question of whether life needs to evolve on the planet or be imported from a passing asteroid. Page 2: Zone of Liquid Water Possibility Q. If a pla ...
Sparta High School
Sparta High School

Starlight and What it Tells Us
Starlight and What it Tells Us

... 100 x 100 = 10,000 times brightness distance Sirius and the Pup are same color, therefore same temperature (Pup is hotter) • Pup must have 1/10,000 the apparent area of Sirius = 1/100 the diameter ...
Chapter 1 - A Modern View of the Universe
Chapter 1 - A Modern View of the Universe

... Distance Units and Astronomy Planets: kilometers (km) (1 km ~ 0.6 mile) - i.e., Earth’s circumference is ~40,000 km Solar System: Astronomical Unit (AU) - average Earth-Sun distance = 150 million km - Venus is 0.7 AU from Sun, Mars at 1.5 AU Stars, Galaxies, Universe: light year (ly) - 9.46 trillio ...
Stars Unit
Stars Unit

... Apparent Absolute Magnitude Magnitude What the star looks like from Earth… based on distance from earth ...
A Decade in the Life of the Massive Black-Hole Binary... Silas Laycock !
A Decade in the Life of the Massive Black-Hole Binary... Silas Laycock !

... •  Chandra and XMM-Newton data were analyzed separately, yielding two sets of flux-minima, most of which are mutually exclusive. •  The resulting best period, also found by the Lomb-Scargle periodogram, is 125431s (1.45175(1) d) •  Visual inspection confirms no other trial-period can simultaneously ...
Lesson 1 – Explain – Page 375 “The Structure of
Lesson 1 – Explain – Page 375 “The Structure of

...  There could be as many as 1 trillion comets orbiting the Sun. The Astronomical Unit  Objects in the solar system are so far apart that astronomers use a larger distance unit.  An astronomical unit (AU) is the average distance from Earth to the Sun --- about 150 million km. The Motion of the Plan ...
Sample Exam 3
Sample Exam 3

... 19) Tiny quantum fluctuations in the energy density of the universe at 10-33 s after the Big Bang are actually responsible for the later A) expansion of the universe. B) widespread existence of matter, instead of anti-matter or no matter, in the universe. C) formation of large scale structure of the ...
M - UC Berkeley Astronomy w
M - UC Berkeley Astronomy w

Lecture101602
Lecture101602

... how we see most objects in this room how we see planets, the Moon, asteroids, etc glow of hot materials or from fusion how the Sun glows how we see comets ...
RED GIANTS
RED GIANTS

... • Stars are like people in that they are born, grow up, mature, and die. • A star’s mass determines what life path it will take. • We will divide all stars into three groups: ...
distant stars nearby star parallax angle The principle of geometrical
distant stars nearby star parallax angle The principle of geometrical

... Does the star Vega in Lyra appear exceptionally bright because it’s an intrinsically bright star, or simply because it’s unusually close by? What about Betelgeuse in Orion? If we didn’t know the distances to these stars, we wouldn’t know that Betelgeuse is a red giant star, with a much greater intri ...
Unit 3 - Section 8.9 Life of Stars
Unit 3 - Section 8.9 Life of Stars

What`s Out There? - Queen`s University
What`s Out There? - Queen`s University

... Splitting Light into Colours ...
Stars - Stallion Science
Stars - Stallion Science

3.1 Introduction
3.1 Introduction

... In the case of a halo globular cluster, with little foreground contamination, the density of points in the HR diagram approximately reflects the length of time a star spends in different evolutionary stages. Stars spend most of their lives on the main sequence (MS), burning hydrogen in their cores. ...
PRIMARY SOURCE from Starry Messenger
PRIMARY SOURCE from Starry Messenger

... It is a very beautiful thing, and most gratifying to the sight, to behold the body of the moon, distant from us almost sixty earthly radii, as if it were no farther away than two such measures—so that its diameter appears almost thirty times larger . . . as when viewed with the naked eye. In this wa ...
AST 301 Introduction to Astronomy - University of Texas Astronomy
AST 301 Introduction to Astronomy - University of Texas Astronomy

... When the Sun becomes a red giant, its radius will increase to about ½ AU, and it will become more than 100 times more luminous than it is now. Life will not be pleasant on Earth. The core of the Sun will be mostly helium, and will continue to contract and heat up. When the temperature in the core re ...
The Sky is Our Laboratory
The Sky is Our Laboratory

... galaxies? 16. How many different types of galaxies are there? • It is called the `bulge’ and it consists of stars, generally fairly old. Most galaxies have bulges.. For instance, elliptical galaxies could be considered to consist entirely of a `bulge’. Most spiral galaxies have bulges. There is a (n ...
Planets around Other Stars - Sierra College Astronomy Home Page
Planets around Other Stars - Sierra College Astronomy Home Page

... The period between transits (3.5 days) exactly matched what was derived with the Doppler method. The mass, radius (and therefore volume) were derived allowing us to calculate a density. This density was consistent with a Jovian planet. Atmospheric information could be derived too. © Sierra College A ...
NGC 3370 Spiral Galaxy
NGC 3370 Spiral Galaxy

... forming. O,B,A,F,G,K,M • Spiral arms barely move, but gas clouds and stars orbit around the galaxy moving in and out of spiral arms • From the HR diagram, by far the most luminous stars are the O-type stars. Their luminosity can be 100,000 times the Sun’s. • Why is the spiral structure in galaxies s ...
Starlight & Stars - Wayne State University Physics and Astronomy
Starlight & Stars - Wayne State University Physics and Astronomy

... Brightness of Stars (1) The total amount of energy at all wavelengths that a star emits is called its luminosity Note: this is how much energy the star gives off each second, NOT how much energy ultimately reaches our eyes or telescope The luminosity of a star is perhaps its most important characte ...
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