![tutorial #10 [wave nature of light] .quiz](http://s1.studyres.com/store/data/020410144_1-db052accb2aa8cded167524d89755606-300x300.png)
B/W
... Sun and interstellar medium Typically: Hydrogen 90% by number; Helium 10%; other elements (metals) ¿ 1 % (by mass: X ' 0.70, Y ' 0.28, Z ' 0.02) • Globular cluster stars: Metal deficient compared to Sun by factors of 10 – 1000, Hydrogen and helium normal Assuming uniform initial composition for the ...
... Sun and interstellar medium Typically: Hydrogen 90% by number; Helium 10%; other elements (metals) ¿ 1 % (by mass: X ' 0.70, Y ' 0.28, Z ' 0.02) • Globular cluster stars: Metal deficient compared to Sun by factors of 10 – 1000, Hydrogen and helium normal Assuming uniform initial composition for the ...
Note
... • The observed profile is the convolution of the true line profile with the instrument profile • For high S/N ratio data, Fourier techniques can be used to back out the IP from a spectrum to recover some of the resolution. ...
... • The observed profile is the convolution of the true line profile with the instrument profile • For high S/N ratio data, Fourier techniques can be used to back out the IP from a spectrum to recover some of the resolution. ...
How Common is Life in the Milky Way?
... Indicate how common you believe intelligent civilizations are in the Milky Way Galaxy: ...
... Indicate how common you believe intelligent civilizations are in the Milky Way Galaxy: ...
Standard 1-1.A “The Big Bang Theory” Study Notes
... Light from stars support the Big Bang Theory because it shows that most objects in space are moving away from one another. 2. The spectrum of hydrogen on a distant star is red shifted. 3. Stars farthest from Earth with the greatest speed have the greatest red shift. 4. Scientists accept the Big Bang ...
... Light from stars support the Big Bang Theory because it shows that most objects in space are moving away from one another. 2. The spectrum of hydrogen on a distant star is red shifted. 3. Stars farthest from Earth with the greatest speed have the greatest red shift. 4. Scientists accept the Big Bang ...
Pre-test on THE UNIVERSE, GALAXIES, AND STARS
... 9. if the nearest star is 4.2 light-years away then • the light we see left the star 4.2 years ago. • the star is 4.2 million miles away. • the star must have formed 4.2 billion years ...
... 9. if the nearest star is 4.2 light-years away then • the light we see left the star 4.2 years ago. • the star is 4.2 million miles away. • the star must have formed 4.2 billion years ...
1)2 A light year is a) about six trillion miles. b) the distance to the star
... a) heat within the Earth that is left over from formation and created by radioactive decay. b) heat from the sun being absorbed by the surface. c) the moon's tidal forces. 11)2 Evidence from Type I A supernovae indicates that a) our galaxy is expanding b) the local group of galaxies is expanding c) ...
... a) heat within the Earth that is left over from formation and created by radioactive decay. b) heat from the sun being absorbed by the surface. c) the moon's tidal forces. 11)2 Evidence from Type I A supernovae indicates that a) our galaxy is expanding b) the local group of galaxies is expanding c) ...
THE HISTORY OF THE UNIVERSE IN ONE EASY LESSON
... “Astronomy is more than the study of stars and planets. It is the study of the universe in which we humans exist. You and I live on a small planet circling a small sun drifting through the universe, but astronomy can take us beyond these boundaries and help us not only see where we are in the univer ...
... “Astronomy is more than the study of stars and planets. It is the study of the universe in which we humans exist. You and I live on a small planet circling a small sun drifting through the universe, but astronomy can take us beyond these boundaries and help us not only see where we are in the univer ...
Stars & Galaxies
... stars that have less mass than the sun use their fuel slowly, and can live for about 200 billion years. Medium- mass stars like the sun live for about 10 billion years. ...
... stars that have less mass than the sun use their fuel slowly, and can live for about 200 billion years. Medium- mass stars like the sun live for about 10 billion years. ...
Relative sizes of astronomical objects
... largest known star. It is between 1,800–2,100 times the diameter of the Sun. Placed at the center of our solar system, its diameter would extend out slightly beyond the orbit of Saturn. ...
... largest known star. It is between 1,800–2,100 times the diameter of the Sun. Placed at the center of our solar system, its diameter would extend out slightly beyond the orbit of Saturn. ...
the life cycle of stars
... • Energy is generated in the core and causes the star to shine. • The size of the star changes very little as long as its supply of hydrogen nuclei fuse into helium nuclei. ...
... • Energy is generated in the core and causes the star to shine. • The size of the star changes very little as long as its supply of hydrogen nuclei fuse into helium nuclei. ...
DUST FROM EVOLVED STARS TO PROTOSTARS. A. K. Speck
... molecules [e.g. 5]. Furthermore, dust has been observed at higher redshifts than expected, and understanding this phenomenon is vital to our understanding of the cosmos at large and its evolution [e.g. 6, 7].Such a crucial and ubiquitous constituent of our Universe needs to be well understood in its ...
... molecules [e.g. 5]. Furthermore, dust has been observed at higher redshifts than expected, and understanding this phenomenon is vital to our understanding of the cosmos at large and its evolution [e.g. 6, 7].Such a crucial and ubiquitous constituent of our Universe needs to be well understood in its ...
Gravitational redshift of Sirius B Equivalent velocity 80 km/s
... Equivalence principle – this situation should be the same ...
... Equivalence principle – this situation should be the same ...
QntmEx
... Most of the northern lights we see form in the ionosphe re. The energy of solar wind is converted to visible light by a mechanism called a quantum leap. To explain a quantum leap, imagine a hydrogen atom consisting of a single positive proton nucleus around which spins a single elec tron at a set d ...
... Most of the northern lights we see form in the ionosphe re. The energy of solar wind is converted to visible light by a mechanism called a quantum leap. To explain a quantum leap, imagine a hydrogen atom consisting of a single positive proton nucleus around which spins a single elec tron at a set d ...
Scientific Notation Introduction Activity
... Click the manual button to stop the automatic display. Use the increase and decrease arrows to find the sizes below. Fill in the chart below for the following views: [you will have to ‘wrap’ the zeros for the larger numbers] ...
... Click the manual button to stop the automatic display. Use the increase and decrease arrows to find the sizes below. Fill in the chart below for the following views: [you will have to ‘wrap’ the zeros for the larger numbers] ...
PPT
... below? Do you think its’ orbit around the sun is more or Less elliptical as compared to Earth? ...
... below? Do you think its’ orbit around the sun is more or Less elliptical as compared to Earth? ...
Slide 1
... Most of the elements with second ionization potentials close to 13.6 eV exhibit lower abundances than the other elements. It can be the sign of charge-exchange reactions in the atmosphere of PMMR 144 It can be the result of higher density of interstellar medium in SMC ...
... Most of the elements with second ionization potentials close to 13.6 eV exhibit lower abundances than the other elements. It can be the sign of charge-exchange reactions in the atmosphere of PMMR 144 It can be the result of higher density of interstellar medium in SMC ...
I`m using this stupid huge font
... experiences its timeline, other parts of the global space-time (other universes) can live through their own lifetimes, as part of a cosmic archipelago sometimes called the ...
... experiences its timeline, other parts of the global space-time (other universes) can live through their own lifetimes, as part of a cosmic archipelago sometimes called the ...
File - Prairie Science
... When this happens two neutrons are released. Now 2 proton/2 neutron Helium atom. ...
... When this happens two neutrons are released. Now 2 proton/2 neutron Helium atom. ...
Astronomical spectroscopy
Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.