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Stars in the night Sky - ScienceEducationatNewPaltz
Stars in the night Sky - ScienceEducationatNewPaltz

... Find north by using the Big Dipper to locate Polaris, the north star. Polaris is closer to true north than a magnetic compass. o Note: In Japan, azimuth is measured clockwise starting from the south. The point directly overhead is called an observer's zenith. Opposite the zenith is the nadir, direct ...
The Night Sky This Month - Usk Astronomical Society
The Night Sky This Month - Usk Astronomical Society

... above the horizon at sunset so observe Saturn as soon as you can this month, in the south-west. Uranus is at opposition on the 15th and is visible throughout the night this month. At a magnitude of 5.70 it may well be seen with binoculars. A small telescope might show a blue hue, but since Uranus us ...
AST1100 Lecture Notes
AST1100 Lecture Notes

... another another possibility: spectral classes. Stars are classified according to their spectral class which consists of a letter and a number. This historical classification is based on the strength of different spectral lines found in the spectra of the stars. It turned out later that these spectra ...
11 - Visual Magnitudes Project
11 - Visual Magnitudes Project

Brightness and Distance
Brightness and Distance

October 2012 - astronomy for beginners
October 2012 - astronomy for beginners

... Very few constellations look like the characters after which they are named. Cygnus the Swan, Leo the Lion and Orion the Hunter are perhaps exceptions and do (with a little imagination) look remotely like those characters. The stars making up the constellations are not generally physically associate ...
Virgo constellation
Virgo constellation

Observing the Night Sky - Constellations
Observing the Night Sky - Constellations

... location on the Earth and to see the celestial sphere move overhead. The Celestial Sphere Ancient astronomers believed that the Earth was at the center of an enormous Celestial Sphere, to which the stars, Sun, Moon and planets were fixed. For purposes of finding one's way around the sky, this simple ...
1 pracovni list HR diagram I EN
1 pracovni list HR diagram I EN

THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting
THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting

... elements to burn at even higher temperatures, and causing sun-like stars to grow into red giants. Even though the cores of both hydrogen-burning and helium-burning stars have consistent, steady energy outputs, our sun's overall brightness varies by just ~0.1%, while red giants can have their brightn ...
Lecture 10: The Hertzsprung
Lecture 10: The Hertzsprung

Stars - WhatisOutThere
Stars - WhatisOutThere

... brighter than the faint glow coming from the stars. If you were standing on the moon for example, you would be able to see the stars both day and night. This is because there is no atmosphere on the moon, meaning that it is always dark. Therefore you can see the stars. ...
Binocular Universe: Summer`s Swan Song
Binocular Universe: Summer`s Swan Song

CONSTELLATIONS
CONSTELLATIONS

1. What is parallax? What unit is it measured in? 1a. Parallax is the
1. What is parallax? What unit is it measured in? 1a. Parallax is the

Transcript - Chandra X
Transcript - Chandra X

... are more diverse and complicated than this diagram would lead you to believe. For instance, there are many more stellar classes than OBAFGKM; however for simplicity’s sake, only the classes that contain a large majority are shown. Absolute magnitude – the intrinsic brightness of stars – is similar ...
Measuring the Properties of Stars - Sierra College Astronomy Home
Measuring the Properties of Stars - Sierra College Astronomy Home

Week8Lecture1
Week8Lecture1

Student Exploration Sheet: Growing Plants
Student Exploration Sheet: Growing Plants

Polaris
Polaris

... about 2400 AU (360 billion kilometers, or 224 billion miles). Polaris B can be seen with even a modest telescope and was first noticed by William Herschel in 1780. In 1929, it was discovered by examining the spectrum of Polaris A that it had another very close dwarf companion (variously α UMi P, α U ...
Lesson 4. Wiens and Stefans Laws
Lesson 4. Wiens and Stefans Laws

Galaxies and Stars
Galaxies and Stars

Mass and the Properties of Main Sequence Stars
Mass and the Properties of Main Sequence Stars

Measuring Distances
Measuring Distances

Lecture 3
Lecture 3

... • The parallax effect is the apparent motion of a nearby object compared to distant background objects because of a change in viewing angle. • Put a finger in front of your nose and watch it move with respect to the back of the room as you look through one eye and then the other. ...
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Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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