Slide 1 - Physics @ IUPUI
... rotations (seconds) • Only seem to last 10,000 years or so • Hard to observe flare up only very randomly ...
... rotations (seconds) • Only seem to last 10,000 years or so • Hard to observe flare up only very randomly ...
Lesson #5: Constellations - Center for Learning in Action
... In the center of the black circle, draw the points (stars) of the constellation each student chose. Use a pin or the point of a sharpened pencil to punch a small hole through each of the drawn points (stars). Wrap the circle over the tube and secure it with a rubber band. Look through the tube at a ...
... In the center of the black circle, draw the points (stars) of the constellation each student chose. Use a pin or the point of a sharpened pencil to punch a small hole through each of the drawn points (stars). Wrap the circle over the tube and secure it with a rubber band. Look through the tube at a ...
The Hertzsprung-Russell Diagram
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
THE HR DIAGRAM
... relative quantities. To create a general HR diagram, many stars are observed at a given time, their luminosity and temperature are determined and those values are plotted. The HR diagram can be thought of as a snapshot plot of these stars at one time. A star's position on the HR diagram is determine ...
... relative quantities. To create a general HR diagram, many stars are observed at a given time, their luminosity and temperature are determined and those values are plotted. The HR diagram can be thought of as a snapshot plot of these stars at one time. A star's position on the HR diagram is determine ...
Name _________ Date _____________ Period ______ Skills
... _____ 26. What unit of measurement do astronomers use to measure the distance from Earth to the stars? a. a solar year b. a parallax c. a light-year d. magnitude 27. The distance that light travels in one year; about 90.46 trillion kilometers, is called a(n) ______________________. 28. An apparent s ...
... _____ 26. What unit of measurement do astronomers use to measure the distance from Earth to the stars? a. a solar year b. a parallax c. a light-year d. magnitude 27. The distance that light travels in one year; about 90.46 trillion kilometers, is called a(n) ______________________. 28. An apparent s ...
Document
... the Greeks rejected the heliocentric theory because they did not • Example: detect stellar parallax. Tycho later realized that this is because stars are too far away to measure with current precision. ...
... the Greeks rejected the heliocentric theory because they did not • Example: detect stellar parallax. Tycho later realized that this is because stars are too far away to measure with current precision. ...
Characteristics of Stars
... nuclear fusion is happening at their cores… they create their own light • Have different characteristics which allow many different ‘varieties’ of stars to exist ...
... nuclear fusion is happening at their cores… they create their own light • Have different characteristics which allow many different ‘varieties’ of stars to exist ...
WebQuest-The-Life-Cycle-of-Stars-1
... and see pictures of the protostars of M16: The Eagle Nebula and other nebulae on this page. Continue by reading up on Main Sequence Stars and find out how our sun compares in mass to other stars. 1) Compare the mass of our sun to Sirius? To Proxima Centauri? 2) Based on its mass, will our sun be aro ...
... and see pictures of the protostars of M16: The Eagle Nebula and other nebulae on this page. Continue by reading up on Main Sequence Stars and find out how our sun compares in mass to other stars. 1) Compare the mass of our sun to Sirius? To Proxima Centauri? 2) Based on its mass, will our sun be aro ...
3-Stars AM Adapted - vhs-ees-am
... type of death for Massive and Giant Blue Stars. They are a ...
... type of death for Massive and Giant Blue Stars. They are a ...
Life Cycles of Stars
... • At least 10 times the size of our Sun • When a high mass star runs out of fuel it collapses and expands to form a Supergiant • Supergiants end in a massive explosion called a supernova • End result: 1) cosmic debris - nebula 2) a neutron star (or pulsar) 3) a black hole ...
... • At least 10 times the size of our Sun • When a high mass star runs out of fuel it collapses and expands to form a Supergiant • Supergiants end in a massive explosion called a supernova • End result: 1) cosmic debris - nebula 2) a neutron star (or pulsar) 3) a black hole ...
From the Everett and Seattle Astronomical
... familiar asterism of three stars. Vega is also one of three brilliant stars that divide the northern heavens into thirds, the others being Arcturus and Capella. At magnitude zero, Vega is the sky's fifth brightest star. Epsilon Lyrae, one of the most observed multiple star systems, is easy to find i ...
... familiar asterism of three stars. Vega is also one of three brilliant stars that divide the northern heavens into thirds, the others being Arcturus and Capella. At magnitude zero, Vega is the sky's fifth brightest star. Epsilon Lyrae, one of the most observed multiple star systems, is easy to find i ...
Variable and Binary Stars
... By a small majority, all stars are binary or trinary – 53% of star systems are multiple – 75% of O-type stars seem to have a companion – If Jupiter had been ~100 times more massive, the Sun would have a companion star ...
... By a small majority, all stars are binary or trinary – 53% of star systems are multiple – 75% of O-type stars seem to have a companion – If Jupiter had been ~100 times more massive, the Sun would have a companion star ...
- hoganshomepage
... Spectroscope: Used to measure the chemical composition of the stars. (also temperature and direction the star is moving in relation to the Earth.) How? Set up a spectroscope with different tubes; each gas has different spectras – light patterns. ...
... Spectroscope: Used to measure the chemical composition of the stars. (also temperature and direction the star is moving in relation to the Earth.) How? Set up a spectroscope with different tubes; each gas has different spectras – light patterns. ...
Startalk
... How are they born how do they die? PHOTO COURTESY NASA The constellation Orion as seen from the space shuttle Endeavour (STS-54) ...
... How are they born how do they die? PHOTO COURTESY NASA The constellation Orion as seen from the space shuttle Endeavour (STS-54) ...
Classifying Stars - Concord Academy Boyne
... The Hertzsprung-Russell Diagram The H-R Diagram shows the relationship between absolute magnitude, luminosity, classification, and effective temperatures of stars. It is a graph that plots star color versus its luminosity. The H-R Diagram can be used to define different types of stars. ...
... The Hertzsprung-Russell Diagram The H-R Diagram shows the relationship between absolute magnitude, luminosity, classification, and effective temperatures of stars. It is a graph that plots star color versus its luminosity. The H-R Diagram can be used to define different types of stars. ...
Distance to Stars
... 40 trillion km from the sun. (more than 260,000AU) • Light takes 4.2 years to reach Earth. ...
... 40 trillion km from the sun. (more than 260,000AU) • Light takes 4.2 years to reach Earth. ...
Stars Power Point
... • Low numbers are brightest, high are dimmest • Sun = -26.7 • Sirius = -1.45 (Brightest Star) ...
... • Low numbers are brightest, high are dimmest • Sun = -26.7 • Sirius = -1.45 (Brightest Star) ...
Constellations 1
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
Constellations 1
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
constellations[1]
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
... night long and all year long. It seems that these stars do not rise and set, but circle the Earth’s north pole each night. These stars are called circumpolar. ...
Astro 1 & 100 Levine Homework Stars Name:____________________________
... You may want to do the lecture-tutorial on pg 33, Apparent and Absolute Magnitude of Stars, prior to doing this portion of the homework, if you need a refresher on m and M. Ranking questions are 2 points each. Consider the following table of stars: ...
... You may want to do the lecture-tutorial on pg 33, Apparent and Absolute Magnitude of Stars, prior to doing this portion of the homework, if you need a refresher on m and M. Ranking questions are 2 points each. Consider the following table of stars: ...
Star catalogue
A star catalogue, or star catalog, is an astronomical catalogue that lists stars. In astronomy, many stars are referred to simply by catalogue numbers. There are a great many different star catalogues which have been produced for different purposes over the years, and this article covers only some of the more frequently quoted ones. Star catalogues were compiled by many different ancient peoples, including the Babylonians, Greeks, Chinese, Persians, and Arabs. Most modern catalogues are available in electronic format and can be freely downloaded from NASA's Astronomical Data Center.Completeness and accuracy is described by the weakest apparent magnitude V (largest number) and the accuracy of the positions.