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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

... b) A star is found to have a displacement on the plates of almost half a pixel - 10 microns due to parallax, and simultaneously has a yearly displacement of 20 microns due to proper motion. Find its annual proper motion, its distance, and its transverse velocity. c) For this same star, a heliocentri ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • Stars range from .0001xLS to 1,000,000xLS Another scale: “magnitude” often used. A log scale to the power of ~2.5. YOU DON’T NEED TO KNOW. The lower the Mag the brighter the object PHYS 162 ...
Lecture 11
Lecture 11

... • Common units for proper motions (which are typically very small) are milliarcseconds/year (mas/yr) • By the above equation, we see that a proper motion can be large if: – the star has small distance, d – the star has a large transverse velocity with respect to the Sun ...
PPT - Yale University
PPT - Yale University

... formation of compact objects by transporting angular momentum.  The formation of objects like stars and black holes is then a much more complex, dynamic, and chaotic process than in standard models.  Gravitational interactions tend to couple the mass of a forming object to the mass of the system, ...
intro.phys.psu.edu
intro.phys.psu.edu

... ❖ The path of the planets about the sun is elliptical in shape, with the center of the sun being located at one focus.---- Kepler's First Law, also The Law of Ellipses ❖ An imaginary line drawn from the center of the sun to the center of the planet will sweep out equal areas in equal intervals of ti ...
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... 1. The small inhabitable zone that is around a star is hard for planets to be found in and is rare to see them in this location 2. Another idea is that the solar system must consist of planets like ours, small rocky planets near the star and large gas giants on the outer rim. 3. Having a consistent ...
Chapter 3 Cosmology 3.1 The Doppler effect
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... Astronomers in 1998 studying type Ia supernovae were astounded when they discovered very distant supernovae much further away than expected. To reach such distances, the supernovae must have been accelerating. The astronomers concluded that the expansion of the Universe is accelerating and has been ...
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Fermi Quiz Instructions

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Phys 1533 Descriptive Astronomy

... • Equinoxes - two points where the ecliptic intersects the celestial equator. The day and night are of equal length at these two points. • Autumnal equinox - on September 21. • Vernal equinox - on or near March 21. • One tropical year - the interval of time from one vernal equinox to the next (365.2 ...
society journal - Auckland Astronomical Society
society journal - Auckland Astronomical Society

... summer night sky and as it gets dark outside we will move to telescope viewing. The EWB Zeiss Telescope will be available for viewing as well as portable telescopes outside in the courtyard. Ivan Vazey (AAS Curator) will be on hand to help people who have questions about telescopes or your own teles ...
Basic Astronomy Note - Mr. Dewey – Grade 7/8
Basic Astronomy Note - Mr. Dewey – Grade 7/8

... the Earth), and days are shorter during the winter months (our time in the sunshine is shorter during each rotation of the Earth). On the first day of summer (summer solstice), the sun at noon is directly overhead at locations along the Tropic of Cancer (the line on the globe 23.5 degrees north of t ...
the printable Observing Olympics Object Info Sheet in pdf
the printable Observing Olympics Object Info Sheet in pdf

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... 23½ o tilt of the Earth's celestial equator with respect to the ecliptic (the path of the sun through the fixed stars). This will occur twice a year as the sun passes through the zenith and then back, except at the two tropic latitudes when it will occur once a year. 6. What is a penumbral eclipse o ...
Parallax and Its role In the helIocentrIc/GeocentrIc debate
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Starry Night Lab
Starry Night Lab

... 10. Set for 9 pm, 10 days in the future. Where is the constellation you found before (higher or lower)? Go to 9 pm, 20 days from now and see where the constellation is now. 11. Summarize what you've just found: (circle the right answer) A given star rises 4 minutes [earlier/later] each night. We cal ...
chapter 7 review questions
chapter 7 review questions

... Stars of this temperature are too cool to produce an absorption spectrum. ...
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Stellar Interiors - Hydrostatic Equilibrium and Ignition on the Main

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QDSpaperFred1.tex

... This is a consequence of the second law of thermodynamics.) Since any given thermal technology should have an optimal temperature, artificial emissions should be closer to black body radiation. Thus, high spectral resolution data between 10-20 microns, as is available from the Keck infrared instrume ...
Magnitudes lesson plan
Magnitudes lesson plan

... that he could see from his latitude into six classes of brightness. His idea of six classes probably came from the Babylonians whose base number was six. The formal introduction of six magnitudes has been credited to Ptolemy (100-150 A.D.) who was a Greek/Egyptian astronomer. He simply advanced the ...
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... In these layers we have an intricate web of different processes occurring and interacting in the same region and in the same time scale: convection, magnetic fields and pulsations. Beneath the stellar surface (a few percent of the star’s radius) this interaction becomes even more complicated due to ...
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Ay123 Homework 1 Solutions

... a What is the angular size of each of the stars and of the semi-major axis? If you can measure angles on the sky with a 1σ rms accuracy of 0.01 arcsec, what is the percentage accuracy of the measurement of the semi-major axis and of the radius of each star? From the parallax, we know d = 10 pc = 3 × ...
Chapter 12
Chapter 12

... Analyzing the HR Diagram • The Stefan-Boltzmann law is a key to understanding the H-R diagram – For stars of a given temperature, the larger the radius, the larger the luminosity – Therefore, as one moves up the H-R diagram, a star’s radius must become bigger – On the other hand, for a given lumino ...
Physics 121 - Spring 2001
Physics 121 - Spring 2001

... b) Now, suppose you want this object to have a speed of 100 m/s when it reaches infinity, instead of coming to rest at infinity. What should the initial speed be in this case? 3. In 1920, a prominent newspaper editorialized as follows about the pioneering rocket experiments of Robert H. Goddard, dis ...
11 - Visual Magnitudes Project
11 - Visual Magnitudes Project

... Attached is a finding chart for the brighter stars in the open star cluster named Praesepe or M44 which lies in the constellation of Cancer, or Pleiades (M45) which lies in the constellation of Taurus. M44 and M45 are the 44th and 45th objects in the catalog compiled by Messier. Visual photometry is ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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