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Brightness + Magnitude of Stars
Brightness + Magnitude of Stars

Stellar Evolution and the HR Diagram – Study Guide
Stellar Evolution and the HR Diagram – Study Guide

... c. Which is brighter, the sun or a white dwarf? The Sun (but not as hot) d. Is Vega brighter than our sun? Yes e. Is Antares hotter than our sun? No, it’s a giant, class K or M 22. Stars that move off the main sequence first move to the _Giant_ region of the HR diagram. These stars are fusing __heli ...
Chapter 28 Stars and Their Characteristics
Chapter 28 Stars and Their Characteristics

... (Volume x Luminosity) and Distance from Observer. Betelgeuse, one of the brightest stars in the Universe, does not appear to be as bright as our Sun, because of its ...
H-R diagram worksheet
H-R diagram worksheet

Linking Asteroids and Meteorites through Reflectance
Linking Asteroids and Meteorites through Reflectance

"Stars" Power Point notes
"Stars" Power Point notes

... brightness of a star as measured on Earth. - Apparent magnitude depends on the star’s actual brightness and distance. - The smaller the magnitude number, the brighter the star. (http://spaceweather.com/flybys ) ...
Star Questions 2008 - Fort Thomas Independent Schools
Star Questions 2008 - Fort Thomas Independent Schools

... Explain what it means for a star to be on the main sequence. Which two pressures act upon any star on the main sequence? Why a star remains roughly the same diameter when on the main sequence. Explain the following relationships: a. Surface temperature and color b. luminosity and mass c. absolute an ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... Laboratory (LBNL). Within minutes, supercomputers subtract reference images from each incoming image, comparing new sources of light to all public databases to tag known variable stars and asteroids. Every night, on average, iPTF discovers one to two new supernovae. Caught in the act Less than 30 mi ...
8.3 Stars
8.3 Stars

... Over a very long time, a white dwarf will cool to temperatures at which it is no longer visible and become a cold black dwarf; become a lump of coal in the sky when all its nuclear energy is gone ...
bYTEBoss lesson 3 life of star
bYTEBoss lesson 3 life of star

... The end of the life cycle of really massive stars is different to that of massive stars. After a really massive red giant collapses in a supernova explosion, it leaves a star so dense that not even light can escape its gravitational pull. This is called a black hole! Some scientists believe that the ...
Branches of Earth Science
Branches of Earth Science

... Light Year- Astronomers use light years to measure the distances ______________ stars o A light year is the distance that light ______________ in one year  9,460,730,472,580.8 km  5,878,630,000,000 miles Parallax- the apparent change in the ______________ of a star in the sky. o The change is due ...
Basic Observations of Stars
Basic Observations of Stars

... changing directions, expressed as angles. This is called the star’s proper motion. (To calculate the actual speeds through space, we need to know their distances as well.) The changes are more noticeable for nearby stars. A nearby object can appear to ‘whiz’ across the sky even if it is moving at mo ...
Stellar Evolution
Stellar Evolution

... uncertain. ...
Constellations
Constellations

... Winter ...
Exploring Space
Exploring Space

Measuring stars Part I
Measuring stars Part I

absolute magnitude
absolute magnitude

File - SMIC Physics
File - SMIC Physics

... • ~ 1 trillion stars • Stars (including Sun) orbit around the core. It takes 225 million years for the Sun to make 1 round around the core. • Has a supermassive black hole at its center. It is about 2.5 million times as massive as the Sun. ...
First Exam - University of Iowa Astrophysics
First Exam - University of Iowa Astrophysics

... 26. You look up in the night sky and see the planet Jupiter, the planet Mars, and the Moon very close together. You know that they are located in or close to one of the following. Which is it? (a) the ecliptic ∗ (b) the celestial equator (c) the zenith (d) the north celestial pole (e) the constellat ...
Lecture 5: Light as a tool
Lecture 5: Light as a tool

... temperature of a red star would be? 2) A blue star has a wavelength of maximum emission at 434 nm. What is the surface temperature of this star? ...
Herzsprung-Russell Diagram
Herzsprung-Russell Diagram

... further means to measure the distance to far away stars in our galaxy (Spectroscopic parallax)  RUNG 4 Procedure: •Determine the star’s spectral type from spectroscopy and measure the star’s apparent brightness. •Use the main sequence to get the star’s luminosity. •Use the Inverse Square Law for Br ...
File
File

... From the list below, choose the term that best completes each sentence and then write the entire sentence in your notebook. spectrograph constellation light-year ...
this article as a PDF
this article as a PDF

Abs-Apar Mag
Abs-Apar Mag

The Life Cycle of the Stars
The Life Cycle of the Stars

... The star-filled sky is in many ways like a large crowd of people. Within that group you may find babies, children, teenagers, adults and even senior citizens. Like humans, stars pass through different stages in their lives. They are born, they mature and, eventually, they die. However, unlike humans ...
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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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