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Powerpoint of lecture 14
Powerpoint of lecture 14

... • Post-MS timescale also nuclear (except for a few phases) – so again much more data than for pre-MS studies • Two kinds of observational constraint  Statistical studies of large numbers of field stars (problem: selection effects, e.g. more luminous stars dominate sample)  Look at star clusters: s ...
Measuring the Stars pages 813-820
Measuring the Stars pages 813-820

... west, because of the revolution of the Earth around the Sun. ...
A bowshock model for the wind-ISM interaction of the run
A bowshock model for the wind-ISM interaction of the run

... WR 124 is a galactic Wolf-Rayet star of spectral type WN8, with a mass of about 20 M and a luminosity of 6 105 L [1]. The star is at a distance of about 6.5 kpc and moves away from us with 200 km s 1 . Around the star, the clumpy nebula M1-67 is seen (see Figure 1), believed to be ejected from the s ...
April 2006 Newsletter PDF - Cowichan Valley Starfinders Society
April 2006 Newsletter PDF - Cowichan Valley Starfinders Society

... divided into twelve 30o segments, approximately fitting the constellations of the Zodiac that loop around this circle. During the time of the Babylonians, the equinox occurred in the first degree of Aries and horoscopes still preserve this fact. In the meantime, a few thousand years later, the equin ...
Stars
Stars

... The brightest star in the sky (besides the Sun) is Sirius. It is 2.6 pc from Earth. How long does it take light from Sirius to reach us? ...
Summary of the Presentation
Summary of the Presentation

... (assuming a constant production rate) eliminating 2/3 as being too young, the value of R was estimated to be ~85,000 suitable stars per billion cubic light years. Of the stars examined for planets, planets have been found around only ~12%. As the ability to detect small planets improves, a larger pe ...
PH507-assn-exo-answers
PH507-assn-exo-answers

... Assignment 4 : SMITH 1. Suppose that two exoplanets are observed to transit the same star. They are both in circular orbits with an inclination of 90 degrees. One produces periodic dips with a period of 4 days and the other produces periodic dips with a period of 108 days. The decrease in luminosity ...
General Astronomy - Stockton University
General Astronomy - Stockton University

... We can infer distance from parallax using the slight apparent shifts in relative position ...
Chapter 15, Galaxies
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... Because the mass of white dwarfs when they explode as supernovae is always around 1.0 M⊙, its luminosity is very consistent, and can be used as a standard candle for the measurement of distance to distant galaxies (Chapter 15). The amount of energy produced by white dwarf supernovae and massive star ...
Formation of the Solar System
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... • Leftover bodies from planet building in Jovian planet zone. Hence more icy than asteroids. • Oort Cloud and TNOs are sources of comets. For example, a TNO may encounter Neptune and get sent into inner Solar System, where they start to evaporate, grow a tail, and appear as comets. ...
october 2008 - Mahoning Valley Astronomical Society
october 2008 - Mahoning Valley Astronomical Society

... this date you should also find chi Cyg near maximum light of 5.2 magnitude. These are the last good weeks of comfortable weather to hunt down Neptune and Uranus, low in the south in Capricornus and Aquarius, respectively. ...
TAKS Study Guide - Northwest ISD Moodle
TAKS Study Guide - Northwest ISD Moodle

Ch. 21 notes-1
Ch. 21 notes-1

... They contain billions of stars but have little gas and dust. So they cannot form new star. They contain old stars. Irregular Galaxies Some galaxies do not have regular shapes. The Large Magellanic Cloud is an irregular galaxy about 160,000 light-years away from our galaxy. It is one of our clos ...
math behind the calculator
math behind the calculator

... The amount of energy given off by a star is directly related to its mass. For this program we are assuming that the star is a main sequence star, where its energy output is relatively easy to predict. A main sequence star is a star that is in the main part of its life cycle—it is not just becoming a ...
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Kepler 186f - Forum Skylive
Kepler 186f - Forum Skylive

... M dwarfs are known to be highly active early in their life, often producing giant and frequent flares that could scorch planets nearby. The M dwarf stars also gravitationally interact with their planets, causing tides that heat the planet and often cause their rotations to be ‘tidally locked’, which ...
IND 6 - 1 Stars and Stellar Evolution In order to better understand
IND 6 - 1 Stars and Stellar Evolution In order to better understand

Stars, Galaxies, and the Universe Section 1 Section 1
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... from Earth, is caused by the movement of Earth. • The stars seem as though they are moving counterclockwise around a central star called Polaris, the North Star. Polaris is almost directly above the North Pole, and thus the star does not appear to move much. • Earth’s revolution around the sun cause ...
Intro To Astronomy
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... Earth Rotation = Sky Rotation Polaris - The North Star Circumpolar Star - “Around the Pole” star - Does not set below horizon in the sky at a particular latitude Noncircumpolar Star - Rises and sets at some time during the day or night ...
HR Diagram - TeacherWeb
HR Diagram - TeacherWeb

... In the early 1900s, astronomers identified many star characteristics such as color, size, temperature, and luminosity—or how bright a star is. Using the H-R Diagram Gizmo™, you will discover how some of these characteristics are related. Start by moving your cursor over the stars in the Star collect ...
Name: Date:
Name: Date:

... 5. If a star’s spectrum is shifted toward the blue end of the spectrum, (blue shift) which way are the stars moving? ______________________________________________ _________________________________________________________________________ 6. If a star’s spectrum is shifted toward the red end of the s ...
astrocoursespring2012lec4
astrocoursespring2012lec4

... By now we have studied and observed clusters within the disk of our galaxy and in our western sky in the Spring. These clusters are thousand or so light years away. They also are known to be in the active process of star formation. Now it is time to go beyond the disk of the Milky way to observe Glo ...
Pulsar properties - Pulsar Search Collaboratory
Pulsar properties - Pulsar Search Collaboratory

... The millisecond and binary pulsars occupy the lower left part of the diagram.. Discuss possible evolutionary scenario from normal to MSP There are in fact two types Of “recycled pulsars” •P<30 ms with circular orbits •P>20 ms with eccentric orbits It is thought that these evolve from Low-mass X-ray ...
News Release - האוניברסיטה העברית
News Release - האוניברסיטה העברית

... hundred billion radiant stars, such as our sun, which extend across about 50,000 light years. Every galaxy is embedded in a spherical halo made of dark matter that cannot be seen but is detected through its massive gravitational attraction. The exact nature of this matter is still unknown. The galax ...
Binocular Universe: Summer`s Swan Song
Binocular Universe: Summer`s Swan Song

... but he did spot a small clump of starlight a little less than 2° south-southeast of Sadr. Noting its position, he added it as the 29th entry in his famous catalog. Though not one of Messier’s best, M29 is visible through small, hand-supported binoculars as a tiny, rectangular patch of light, with pe ...
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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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