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Astronomy 15 - Problem Set Number 4 1) Suppose one were to
Astronomy 15 - Problem Set Number 4 1) Suppose one were to

... properties of a CCD signal are somewhat similar to those from a photomultiplier, but there are several complicating factors, so a photomultiplier makes a simpler example. Question: Suppose a star delivers about 1000 pulses per second in a photomultiplier attached to a telescope. Assume for now that ...
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Light Rays

... ray a: part of ray light reflects at interface & the rest travels without change in direction . Rays b, c and d: there are both reflection and refraction at interface. ...
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05_Testbank

... 7) Which of the following cannot be described by a field? A) gravitational forces B) electrical forces C) magnetic forces D) radiation pressure Answer: D 8) The frequency of a wave is A) the number of peaks passing by any point each second. B) measured in cycles per second. C) measured in hertz (Hz) ...
Ultrafast Optics: Tools and Techniques
Ultrafast Optics: Tools and Techniques

... between the X-rays that are produced. Typically, an X-ray will be produced at a certain point on the waveform of the driving laser pulse. (See Fig. 2). In any medium, the index of refraction (and thus the velocity of the light wave) will change as a function of the frequency of the light [6, p. 119] ...
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The Mass-Radius Relation for Polytropes The mass within any point

... electron gas (K = 1.2435 × 1015 µ−4/3 cgs) into (16.1.2), and do the math, the total mass of the star becomes MCh = ...
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Jan 2017 - Bays Mountain Park

... January is the start of a new year. We welcome 2017 with open arms. 2016 was a pretty good year, but I’m hoping 2017 will be even better. We could sure use a year of good weather. It would be nice to have about 300 clear nights here. I know I am dreaming but hey, we can dream. I hope everyone had a ...
The Nature of Space and Time
The Nature of Space and Time

... Since pre-history people have gazed into the sky and pondered the nature of the universe All early civilizations studied the stars and the motions of the five naked-eye planets known to them as the “wanderers” They used their observations to tell time, for navigation, to predict the coming of season ...
digital book, stars and planets
digital book, stars and planets

... light peeking out from behind a tree or between two buildings. Or, you may look up and see a huge, round, disk lighting up the sky. It’s the Moon! ...
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April 2017 - Newbury Astronomical Society

... Red Giant. As this star becomes larger its outer region begins to be attracted by the powerful gravity of the White Dwarf companion. Hydrogen is pulled off the red giant and spirals inwards towards the white dwarf and forms a rotating disc. The Hydrogen gas eventually falls on to the surface of the ...
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A CCD Search for Variable Stars of Spectral Type B in the Northern

... period of 0.39912 d (frequency 2.5055 d 1 ) and the amplitudes (half ranges) of 9 mmag and 8 mmag in B and U, respectively (no V amplitude was given). On the strength of these results, Hill (1967) classified the star as a β Cep variable. However, Delgado et al. (1992), from 42 uvby observations obta ...
High resolution spectral self-interference fluorescence microscopy
High resolution spectral self-interference fluorescence microscopy

... The advantage of light microscopy over electron and scanned probe microscopy is the ability to image the interior of biological specimens. Light would be an ideal carrier of microscopic information if it weren’t for the resolution limit. But because of diffraction, standard light microscopes are not ...
Meteors, Asteroids, and Comets (Powerpoint)
Meteors, Asteroids, and Comets (Powerpoint)

... in late October, the last three months have found the coma of Comet 17P/Holmes both expanding and fading. This spectacular composite image shows how the coma and tail of Comet Holmes have changed. Due to Earth's changing vantage point, Comet Holmes, out beyond the orbit of Mars, was seen in November ...
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BPM Blatt 7

... Question a) Why does an optical trap require an objective with a high numerical aperture? Answer a) When a dielectric sphere is placed in a light gradient, the sum of all rays passing through it generates an imbalance in force, tending to push the sphere towards the brighter region of the light. A f ...
ASTR 1101-001 Spring 2008 - Louisiana State University
ASTR 1101-001 Spring 2008 - Louisiana State University

... Nebulae and White Dwarfs are in order. – The shell of gas that is visible in each planetary nebula illustrates that stars have a way of returning material to the interstellar medium that has undergone nuclear processing. – Over time, the hot “central star” of a PN cools to become a white dwarf: • Ap ...
Comets - Earth & Planetary Sciences
Comets - Earth & Planetary Sciences

... • The model is that of a very dirty snowball or dirty iceberg. However, the outer portion of Halley’s comet (visited by Giotto and Vega 1 & 2 s/c in 1986) was found to be very, very dark, a shell of “sludge” left behind as the vapors baked out. • The coma is a cloud of gas which has evaporated from ...
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Lectures 14 & 15 powerpoint (neutron stars & black holes)

... 4.3 and 3.9 Earth masses! Further analysis revealed a third planet with a mass of about that of our moon! And there is evidence that a fourth planet about 100 Earth masses orbits this pulsar with a much larger separation. Q: How can a NS have planets?!? (Recall that NS are created by supernovae, and ...
THE STARS G. Iafrate(a), M. Ramella(a) and V. Bologna(b) (a) INAF
THE STARS G. Iafrate(a), M. Ramella(a) and V. Bologna(b) (a) INAF

... explained before performing the use case. It is required to draw coordinate points on a diagram. The level of the UC is intermediate. ...
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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.
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