Surface Environments of the Planets o+ our Solar System
... In this exercise, you will also become more familiar with the various naming systems for stars. Remember, only the brightest stars which form our constellations have been given proper names. There are thousands of stars that have either Bayer Greek letter names, and even more that have Flamsteed num ...
... In this exercise, you will also become more familiar with the various naming systems for stars. Remember, only the brightest stars which form our constellations have been given proper names. There are thousands of stars that have either Bayer Greek letter names, and even more that have Flamsteed num ...
Stellar evolution
... Evolution of Stars > 8 MSun Higher mass stars evolve more rapidly and fuse heavier elements. Example: 20 MSun star lives "only" ~107 years. Result is "onion" structure with many shells of fusionproduced elements. Heaviest element made is iron. ...
... Evolution of Stars > 8 MSun Higher mass stars evolve more rapidly and fuse heavier elements. Example: 20 MSun star lives "only" ~107 years. Result is "onion" structure with many shells of fusionproduced elements. Heaviest element made is iron. ...
Star in a Box Worksheet - Beginning with solutions
... radius of the Sun and its temperature is about 8000 K. Betelgeuse has 1000 times the radius of the Sun and its temperature is about 3500 K. 1. What stages of their lives are the two stars in? Deneb is between the main sequence and the Hertzsprung Gap. Betelgeuse is between the Hertzsprung Gap and c ...
... radius of the Sun and its temperature is about 8000 K. Betelgeuse has 1000 times the radius of the Sun and its temperature is about 3500 K. 1. What stages of their lives are the two stars in? Deneb is between the main sequence and the Hertzsprung Gap. Betelgeuse is between the Hertzsprung Gap and c ...
Name________________ Astronomy I cans 1. What is the Big Bang
... The dust and gas in a nebula began to spin, then the dust and gas began accreting (gathering) because of gravity ...
... The dust and gas in a nebula began to spin, then the dust and gas began accreting (gathering) because of gravity ...
Extension worksheet – Topic 6 - Cambridge Resources for the IB
... brightness is made difficult by the presence of dust in the interstellar medium. Suggest the effect this has on the measured distance to the star. ...
... brightness is made difficult by the presence of dust in the interstellar medium. Suggest the effect this has on the measured distance to the star. ...
Star Life Cycle
... Within a nebula, there are varying regions when gravity causes this dust and gas to “clump” together. As these “clumps” gather more atoms (mass), their gravitational attraction to other atoms increases, pulling more atoms into the “clump.” ...
... Within a nebula, there are varying regions when gravity causes this dust and gas to “clump” together. As these “clumps” gather more atoms (mass), their gravitational attraction to other atoms increases, pulling more atoms into the “clump.” ...
Light from stars part II
... passing through a cool, low density gas 3) Emission spectrum: result of a low density gas excited to emit light. The Light is emitted at specific wavelengths ...
... passing through a cool, low density gas 3) Emission spectrum: result of a low density gas excited to emit light. The Light is emitted at specific wavelengths ...
Stellar Evolution
... Since Iron doesn’t release energy when it fuses, It needs vast amounts of energy to fuse, so Fusion Stops. The core shrinks rapidly in microseconds. The Outer-layers crash inward superheating the core to billions of degrees. Iron and other elements fuse into heavy metals and The Outer-layer bounce b ...
... Since Iron doesn’t release energy when it fuses, It needs vast amounts of energy to fuse, so Fusion Stops. The core shrinks rapidly in microseconds. The Outer-layers crash inward superheating the core to billions of degrees. Iron and other elements fuse into heavy metals and The Outer-layer bounce b ...
Spectrum a Star….. - SFA Physics and Astronomy
... Mystery Star Properties 1. The star appears as a point of light through a telescope. 2. The absorption lines appear split and move over a 4 day period. 3. The brightness of the star also varies over 4 days. Question: Why do you think the brightness of the star is varying? Answer: This could be an e ...
... Mystery Star Properties 1. The star appears as a point of light through a telescope. 2. The absorption lines appear split and move over a 4 day period. 3. The brightness of the star also varies over 4 days. Question: Why do you think the brightness of the star is varying? Answer: This could be an e ...
Stellar Formation 1) Solar Wind/Sunspots 2) Interstellar Medium 3) Protostars
... off photons in the hydrogen spectrum ex. “Great Nebula” and 30 Doradus home to formation of hot (0 class) stars ...
... off photons in the hydrogen spectrum ex. “Great Nebula” and 30 Doradus home to formation of hot (0 class) stars ...
18.3 NOTES What is magnitude? Objective: Compare apparent
... Without a telescope, you can see about 2000 stars in the night sky. Some appear brighter than others. One way to measure a star’s brightness is by magnitude. The brightness of a star depends on its temperature, size, and distance from Earth. A hot star is usually brighter than a cool star. A large s ...
... Without a telescope, you can see about 2000 stars in the night sky. Some appear brighter than others. One way to measure a star’s brightness is by magnitude. The brightness of a star depends on its temperature, size, and distance from Earth. A hot star is usually brighter than a cool star. A large s ...
GO1_Distrubtion Of Matter In Space
... • Gravity pulls gas and dust in a NEBULA together into a rotating sphere (composed of ~75% H and 23% He) • As more material is drawn into the spinning ball, the mass at its core increases causing the temperature to rise and possibly start to glow (called a pro-star) • As the process continues, heati ...
... • Gravity pulls gas and dust in a NEBULA together into a rotating sphere (composed of ~75% H and 23% He) • As more material is drawn into the spinning ball, the mass at its core increases causing the temperature to rise and possibly start to glow (called a pro-star) • As the process continues, heati ...
Chapter 18 Study Guide
... White dwarf 9. What type of star has a low temperature but a high luminosity? (use H-R Diagram to determine) Red supergiant 10. According to the Hertzsprung-Russell diagram, what relationship exist between the brightness and temperature of a main sequence star? The Hertzsprung- Russell diagram shows ...
... White dwarf 9. What type of star has a low temperature but a high luminosity? (use H-R Diagram to determine) Red supergiant 10. According to the Hertzsprung-Russell diagram, what relationship exist between the brightness and temperature of a main sequence star? The Hertzsprung- Russell diagram shows ...
1. (6 points, 3 for each answer) Planets are easier to detect around
... but knowing this was not part of the question]. There was one point for each of the following: a) Transits were used to measure the radius. b) Bigger planets block more light. c) The observational consequence of this is that a deeper eclipse indicates a larger planet, and so the depth of the eclipse ...
... but knowing this was not part of the question]. There was one point for each of the following: a) Transits were used to measure the radius. b) Bigger planets block more light. c) The observational consequence of this is that a deeper eclipse indicates a larger planet, and so the depth of the eclipse ...
Test 2, November 14, 2016 - Physics@Brock
... 12. Which of the following features determines the resolving power of a telescope? (a) the focal length of the objective. (b) the focal length of the eyepiece. (c) the diameter of the objective. (d) the diameter of the eyepiece. 13. If the focal length of the objective of a telescope is 120 cm and t ...
... 12. Which of the following features determines the resolving power of a telescope? (a) the focal length of the objective. (b) the focal length of the eyepiece. (c) the diameter of the objective. (d) the diameter of the eyepiece. 13. If the focal length of the objective of a telescope is 120 cm and t ...
Types of Stars - WordPress.com
... • The main sequence is a narrow band of stars on the H-R diagram that runs diagonally from the upper left ( bright, hot stars) to the lower right ( dim, cool stars). About 90 percent of stars are on the main sequence, including the Sun. • A star’s position on the main sequence is determined by its i ...
... • The main sequence is a narrow band of stars on the H-R diagram that runs diagonally from the upper left ( bright, hot stars) to the lower right ( dim, cool stars). About 90 percent of stars are on the main sequence, including the Sun. • A star’s position on the main sequence is determined by its i ...