Powerpoint Presentation (large file)
... • Relatively young Population I stars are metal rich; ancient Population II stars are metal poor • The metals (heavy elements) in Population I stars were manufactured by thermonuclear reactions in an earlier generation of Population II stars, then ejected into space and incorporated into a later ste ...
... • Relatively young Population I stars are metal rich; ancient Population II stars are metal poor • The metals (heavy elements) in Population I stars were manufactured by thermonuclear reactions in an earlier generation of Population II stars, then ejected into space and incorporated into a later ste ...
l rest
... EMR and matter interact all the time This means that matter absorbs and emits EMR Often, the means of interaction is the acceleration of an electron. But this is not the only way, and other ways are possible. The details are not crucial now As long as there is a strong interaction, matter and EMR ca ...
... EMR and matter interact all the time This means that matter absorbs and emits EMR Often, the means of interaction is the acceleration of an electron. But this is not the only way, and other ways are possible. The details are not crucial now As long as there is a strong interaction, matter and EMR ca ...
The correct answers are written in bold, italic and underlined. The
... 15. Tritium is a radioactive form of hydrogen in which the nucleus contains one proton and two neutrons. How much more massive is this nucleus than that of ordinary hydrogen? • The same mass because this nucleus is still hydrogen • Three times as massive • Twice as massive 16. Electron transitions b ...
... 15. Tritium is a radioactive form of hydrogen in which the nucleus contains one proton and two neutrons. How much more massive is this nucleus than that of ordinary hydrogen? • The same mass because this nucleus is still hydrogen • Three times as massive • Twice as massive 16. Electron transitions b ...
Planets beyond the solar system
... • Half the mass of Jupiter • Orbits its star in 4.2 days, compared to 4330 days for Jupiter. • Is only 5 million miles from its sun, 1/8 the distance that Mercury is from our Sun. • Destroyed existing theories of planet formation based on our solar system. ...
... • Half the mass of Jupiter • Orbits its star in 4.2 days, compared to 4330 days for Jupiter. • Is only 5 million miles from its sun, 1/8 the distance that Mercury is from our Sun. • Destroyed existing theories of planet formation based on our solar system. ...
Hot-plate model of stars March 14 − Observed properties of stars
... • For nearby stars, use method of parallax. (Read about parallax in 11.1) ...
... • For nearby stars, use method of parallax. (Read about parallax in 11.1) ...
File
... 1. Clearly and briefly explain the Rare Earth Hypothesis The Rare Earth Hypothesis states that it there is small to if not no other intelligent life in the universe. States that we have existed for such a small time with just the right conditions that we if there was other intellectual life that the ...
... 1. Clearly and briefly explain the Rare Earth Hypothesis The Rare Earth Hypothesis states that it there is small to if not no other intelligent life in the universe. States that we have existed for such a small time with just the right conditions that we if there was other intellectual life that the ...
3 Nightly Motions
... If a star is far enough to the north: It will not rise or set at all! Its path will simply carry it around the North Star in approximately 24 hours, always staying above the horizon. ...
... If a star is far enough to the north: It will not rise or set at all! Its path will simply carry it around the North Star in approximately 24 hours, always staying above the horizon. ...
First Exam - University of Iowa Astrophysics
... 26. You look up in the night sky and see the planet Jupiter, the planet Mars, and the Moon very close together. You know that they are located in or close to one of the following. Which is it? (a) the ecliptic ∗ (b) the celestial equator (c) the zenith (d) the north celestial pole (e) the constellat ...
... 26. You look up in the night sky and see the planet Jupiter, the planet Mars, and the Moon very close together. You know that they are located in or close to one of the following. Which is it? (a) the ecliptic ∗ (b) the celestial equator (c) the zenith (d) the north celestial pole (e) the constellat ...
Deep Space Mystery Note Form 2
... During this short interval, a supernova can radiate as much energy as our Sun could emit over its life span. The explosion expels much or all of the star’s material and causes a shock wave into the surrounding interstellar medium. The interstellar medium is the gas and dust that exists between the s ...
... During this short interval, a supernova can radiate as much energy as our Sun could emit over its life span. The explosion expels much or all of the star’s material and causes a shock wave into the surrounding interstellar medium. The interstellar medium is the gas and dust that exists between the s ...
17Nov_2014
... • If enough material accumulates on the white dwarf’s surface, fusion can be triggered, causing a massive ...
... • If enough material accumulates on the white dwarf’s surface, fusion can be triggered, causing a massive ...
Chapter 12
... together they “touch” . They generate the neutron degeneracy pressure The densities reach 100 trillion g/cm3 (at those densities the whole Earth would fit in a football stadium!!) The collapsing neutron ...
... together they “touch” . They generate the neutron degeneracy pressure The densities reach 100 trillion g/cm3 (at those densities the whole Earth would fit in a football stadium!!) The collapsing neutron ...
PowerPoint Presentation - ASTR498E High energy
... The area under consideration must be oriented face-on to lineof-sight to the star In principle, this definition works for any kind of energy emitted by the star… most commonly, we mean e/m radiation Sometimes, it is useful to consider the observed flux in a restricted range of e/m wavelengths (e.g., ...
... The area under consideration must be oriented face-on to lineof-sight to the star In principle, this definition works for any kind of energy emitted by the star… most commonly, we mean e/m radiation Sometimes, it is useful to consider the observed flux in a restricted range of e/m wavelengths (e.g., ...
Can you write numbers in scientific notation
... Can you define the wave properties of light (wavelength, frequency, speed of light)? Do you understand how light can be described as a particle (photon)? Can you make the following calculations if you are given the equations? - energy of an individual photon - luminosity of a star - the wavelength o ...
... Can you define the wave properties of light (wavelength, frequency, speed of light)? Do you understand how light can be described as a particle (photon)? Can you make the following calculations if you are given the equations? - energy of an individual photon - luminosity of a star - the wavelength o ...
Stars Unit
... There are many different types of stars in the Universe… our star… The SUN; is a very average star ...
... There are many different types of stars in the Universe… our star… The SUN; is a very average star ...
12.4 Evolution of Stars More Massive than the Sun
... It can be seen from this H-R diagram that stars more massive than the Sun follow very different paths when leaving the Main Sequence: ...
... It can be seen from this H-R diagram that stars more massive than the Sun follow very different paths when leaving the Main Sequence: ...