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Star Classification Lab
Star Classification Lab

Document
Document

(HR) Diagrams
(HR) Diagrams

... 5. How many sub-types are there in each spectral class? a. For instance, in the range of A type stars, how many A sub-types are there and what are their names? b. Write down the spectral class of the sub-type halfway between K and M. 6. Which is the hottest type of star, O, B, A, F, G, K or M? Circ ...
White Dwarf Stars Near The Earth
White Dwarf Stars Near The Earth

... the “ages” of the white dwarfs on this page, I mean how long they have been white dwarfs, not how long they were main-sequence stars before that.) 40 Eridani B is a member of a triple star system and was once the brightest and most massive of the three, since the other two are relatively cool K-clas ...
Life Cycle of a Star - CullenScience
Life Cycle of a Star - CullenScience

... As the temperature in the shell of the star increases, the outer layers of the star expand. 2. What is a Red Giant? ...
Life Cycle of Stars
Life Cycle of Stars

Characteristics of Stars
Characteristics of Stars

Name
Name

... Explain the life cycle of a massive star staring with its formation to its death. Be sure to use the following terms and give all possible endings: nebula, black hole, supernova, red supergiant, main sequence, interstellar medium, pulsar ...
What is a Star?
What is a Star?

Constellations 1
Constellations 1

... above the North Pole. This star appears in the same place every night all year long.  In the Northern Hemisphere, if you find Polaris you will be able to tell which direction is north. ...
Constellations 1
Constellations 1

... above the North Pole. This star appears in the same place every night all year long.  In the Northern Hemisphere, if you find Polaris you will be able to tell which direction is north. ...
constellations[1]
constellations[1]

Star Life Cycles
Star Life Cycles

... light a star gives off determines the star’s brightness.  Stars close to Earth can appear bright, even if they do not give off much light. Additionally, very bright stars may appear faint if they are far away.  Parallax – the apparent shift in position of an object when ...
SOLUTIONS ASTROPHYSICS – OPTION D 2015-17
SOLUTIONS ASTROPHYSICS – OPTION D 2015-17

... Examples: Stephan-Boltzmann Law ...
What is the net result of the proton-proton chain? a. 2 protons make
What is the net result of the proton-proton chain? a. 2 protons make

... a. All stars in the cluster are the same size and luminosity b. Their combined light makes them much easier to spot from a distance c. Stars in cluster have the same age, similar compositions, and are essentially at the same distance d. Stars in clusters are all relatively young and therefore shine ...
FRIENDS OF THE PLANETARIUM NEWSLETTER April2002
FRIENDS OF THE PLANETARIUM NEWSLETTER April2002

... hottest. Stars are the same; with the hot 30,000 degree stars being a bluish white in colour and the cold stars like Betelgeuse being red. Our yellow sun lies in between with a surface temperature of around 6000 degrees. Despite its size of at least 160 million suns, its mass is only equivalent to s ...
Interstellar clouds
Interstellar clouds

... • White dwarfs have immense gravity, some with the mass of sun and a volume of the earth. ...
Orion
Orion

... Which stars are main sequence stars? Rigel is a true supergiant, blazing white-hot star of intense brilliance and dazzling beauty. Its surface temperature is about 12,000 K and its energy output exceeds that of our Sun by a factor of many thousands; the computed luminosity is something like 57,000 ...
star map looking north january-march
star map looking north january-march

... Our nearest large galaxy – Andromeda – can be seen in the Andromeda constellation. It appears to us as an elongated fuzzy blob. The Andromeda galaxy is so far away that its light takes over two million years to reach us. ...
calculated using stefan`s law
calculated using stefan`s law

Document
Document

...  Notice that the X axis is spaced unevenly, and the number of Kelvins (degrees) between each line is not constant. This because it is a logarithmic scale. For example: each line between 2,000 and 3,000 represents 100 degrees; but each line between 6,000 and 7,000 represents 200 degrees; and differe ...
The Brightness of Stars
The Brightness of Stars

Shapes in the Sky
Shapes in the Sky

Notes: 3.5 STAR EVOLUTION Name: ______ Star
Notes: 3.5 STAR EVOLUTION Name: ______ Star

... Once the star runs out of fuel for good it will be destroyed. Ø A PLANETARY NEBULA is when a Giant star begins to fall apart and the outer layer of gas float out into space. Ø A supernova is big EXPLOSION that happens when a Supergiant runs out of fuel 6. End of Stars Life. (White Dwarf, Neutron S ...
Life of a star - bahringcarthnoians
Life of a star - bahringcarthnoians

... A star’s life begins when clumps of gas and dust come together from it’s own gravity. Gravity pushes these clumps together to make more pressure. Small amounts of gas and dust fizzle out. If the clump is big enough, the centre of the forming star boosts over 10 million degrees Celsius. A nuclear re ...
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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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