• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Project 4: The HR diagram. Open clusters
Project 4: The HR diagram. Open clusters

... luminosity stars. These are the main sequence stars. Our Sun is one of them. There are a few stars that are not in this diagonal strip. There are some low temperature, high luminosity stars - these are called giants and supergiants. The reason they are so ...
The Galaxy Presentation 2011
The Galaxy Presentation 2011

Part 1: If a 10000 K blackbody has a wavelength of peak emission at
Part 1: If a 10000 K blackbody has a wavelength of peak emission at

... Most students didn’t come close to providing this kind of answer even though it was the basis for the Homework 3 assignment of determining spectral types! A typical answer was something like this: “Astronomers measure the color and luminosity of a star to determine its spectral ...
Young Stars
Young Stars

... •Lighter than 0.08 – they don’t get hot enough for fusion •Heavier than 150 – they burn so furiously they blow off ...
Chapter 8 - TeacherWeb
Chapter 8 - TeacherWeb

... A star life cycle: first stage: it is a ball of gas and dust. Gravity pulls the dust and gas together into a sphere. As the sphere becomes denser it becomes hotter. Hydrogen changes to helium by a process called nuclear fusion. When a star dies its materials return to space---sometimes to form new s ...
Early Spring Observing – Millstone News Night Sky
Early Spring Observing – Millstone News Night Sky

... The Beehive contains a larger star population than most other nearby clusters. Under dark skies the Beehive Cluster looks like a nebulous object to the naked eye; thus it has been known since ancient times. We often find it, rather than the constellation it is found in (Cancer). From Wikipedia: The ...
Lecture 10 - University of Minnesota
Lecture 10 - University of Minnesota

... The First Generation of Stars • Astronomers call elements other than hydrogen and helium “metals” – Metallicity is a measure of how much of something is made out of metals ...
2.1 Introduction
2.1 Introduction

... Figure 2.1 shows two examples of star clusters. Star clusters allow us to appreciate directly some of the physical properties of stars for the simple reasons that, to a first approximation, all the stars of a cluster: (i) are at the same distance from the Sun, and (ii) have the same age. NGC 265 (le ...
File - YEAR 11 EBSS PHYSICS DETAILED STUDIES
File - YEAR 11 EBSS PHYSICS DETAILED STUDIES

... about losses as light travelled through gasses or dust clouds. We can also determine the size of a star by its spectrum. To do this we need to know its Luminosity, the amount of energy given off by each unit area, and an accurate surface temperature. ...
18 Throughout history people around the world have looked up at
18 Throughout history people around the world have looked up at

Chapter 09 - The Independent School
Chapter 09 - The Independent School

Stars
Stars

... toward each other by gravity • Many stars orbit each other • More than 50% of stars occur in pairs or multiples. • Binary stars are used to determine the star property most difficult to calculate – It’s mass ...
Nov - Wadhurst Astronomical Society
Nov - Wadhurst Astronomical Society

... month it rises three hours before the Sun and is so bright it is impossible to confuse it with any other astronomical body. Mars still lies in a difficult position for observation from these latitudes. It is in the constellation of Ophiuchus at magnitude +1.2. As I described last month, the shallow ...
AN INTRODUCTION TO THE STARS AND CONSTELLATIONS
AN INTRODUCTION TO THE STARS AND CONSTELLATIONS

Black Hole
Black Hole

... The surface gravity is so high that a 150 pound person would weigh a million tons. You would be squeezed flatter than a piece of paper. The fastest pulsar known has a period of 0.0014 s. The star spins 642 times per second. Dozens of such “millisecond pulsars” are known. More are being discovered. I ...
Milky Way thin disk
Milky Way thin disk

... Age and metallicity • Bulge/bar stars are old: of order 10 Gyr • They are also metal-rich; more so than the disk near the Sun • However, so are inner disk stars ...
Lecture02-ASTA01 - University of Toronto
Lecture02-ASTA01 - University of Toronto

... you only how bright the star is as seen from Earth. • It doesn’t reveal anything about a star’s true power output – because the star’s distance is not known! • There is an “absolute magnitude scale” where we assign magnitudes that the object would have if placed at a certain distance known as 10 par ...
STELLAR STRUCTURE AND EVOLUTION
STELLAR STRUCTURE AND EVOLUTION

colour
colour

Document
Document

...  Chemical composition and surface temperature  Speed and direction of motion using the Doppler Effect  If source of waves is moving towards us, their frequency is shifted upwards  Stars moving towards us are called blue-shifted  If source of waves is moving away from us, their frequency is shif ...
Stellar Evolution Chapter 12
Stellar Evolution Chapter 12

... recent maximum can be used to predict the time of a future maximum. Suppose that you calculate the time of future maximum brightness and then make measurements to observe this maximum. After the correction for Earth's orbital position has been made, you find that the maximum occurred a few minutes l ...
Stellar Evolution - Lick Observatory
Stellar Evolution - Lick Observatory

Astronomy Webquest Part 1: Life of Stars: Go to http://www.odec.ca
Astronomy Webquest Part 1: Life of Stars: Go to http://www.odec.ca

... 1. Stars are born in _______________. When the clouds of interstellar dust and gas pull in gas and start to collapse, the increased heat will cause the atoms to fuse to helium and form ___________________. Click on next. 2. The longest stage of the star, covering almost ______% is in the ___________ ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

GEARS Workshop Monday - Georgia Southern University
GEARS Workshop Monday - Georgia Southern University

< 1 ... 46 47 48 49 50 51 52 53 54 ... 132 >

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.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report