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Exam 03
Exam 03

... 38. What information does the luminosity class of a star provide? A) Brightness: Higher luminosity class indicates a higher apparent magnitude, which actually means a dimmer star as viewed from Earth. B) Temperature: Stars with a higher luminosity class have a higher temperature. C) Mass: The higher ...
Lect07-2-4-09
Lect07-2-4-09

... orbiting Jupiter. To apply Newton’s law in this case we need to use the calculus, which is beyond the scope of this course. The procedure is nevertheless fairly simple. We build a simple model of the galaxy that permits us to compute the orbital velocities of stars at different radii from the center ...
chapter2 - Empyrean Quest Publishers
chapter2 - Empyrean Quest Publishers

... Earth’s orbit It is tilted about 23½° away from the perpendicular The Earth maintains this tilt as it orbits the Sun, with the Earth’s north pole pointing toward the north celestial pole ...
Carter K 1 - Mrs. Anthony`s English 2
Carter K 1 - Mrs. Anthony`s English 2

Lesson 1 – Explain – Page 375 “The Structure of
Lesson 1 – Explain – Page 375 “The Structure of

... whose orbits are close by.  The solar system has eight objects classified as planets. Inner and Outer Planets  The inner planets are Mercury, Venus, Earth, and Mars. These planets are made mainly of solid rocky materials.  The four planets farthest from the Sun are the outer planets. The outer pl ...
Nogami, D. - Subaru Telescope
Nogami, D. - Subaru Telescope

... superflares, 10- 106 times more energetic (1033 - 1038erg) than the largest solar flares (~1032erg). ・ Such stars rotate fast (10 -100 km s-1) and the magnetic fields of a few kG are distributed in large regions on the stellar surface. ...
Hubble`s Law is the relation between the recession velocity of a
Hubble`s Law is the relation between the recession velocity of a

... formation implies that elliptical galaxies were once more efficient then spirals, not the other way around. Also, while population I stars are younger than population II stars, not all (or even most) population I stars are bright blue O stars. Most (like our sun) are plain old mid or low mass stars ...
Life Cycle of a Star notes
Life Cycle of a Star notes

... As the protostar continues to collapse due to gravity, it will attract more atoms and continually increase in mass and density. The increased density and gravity will cause the core temperature to eventually ...
Slide 1
Slide 1

... Low mass stars have lifetimes comparable to the Age of the Universe High mass stars have very short lifetimes, and disappear quickly! ...
A Triple Conjunction
A Triple Conjunction

... supernova, despite its long duration of visibility). The position (southern Aquila) is consistent with having been a nova, although a little further south of the plane of the Milky Way than is normal. The date of its apparition (March 5 BC), coinciding with the best guess as to the date of the birth ...
presentation format
presentation format

... Copernicus, a Polish astronomer, suggested a dramatically different model of  the Solar System, a heliocentric model, with the Sun at the center Copernicus preserved the idea that planets orbited in circular orbits around  the Sun, however. Big debate ensued, between geocentric and heliocentric mode ...
Formation of Solar System
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... ionised in collisions – thus a plasma of ions and free electrons forms. The motion of charged particles creates a magnetic field. The nucleus of the solar nebula thus had a magnetic field associated with it. Matter close to the nucleus was also partially ionised and moved with it. T for disc fell a ...
STAAR Science Tutorial 35 TEK 8.8B: The Sun
STAAR Science Tutorial 35 TEK 8.8B: The Sun

... Sun) is Proxima Centauri, which is about 4.2 light years away from Earth. This is 263,000 times further away from Earth than our Sun. (Our Sun is 0.000016 lightyears away from Earth.) While there are 11 stars within 10 light-years of Earth, most of the other stars visible in the night sky are many t ...
5. cosmic distance ladder ii: standard candles
5. cosmic distance ladder ii: standard candles

... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
The Galactic Super Star Cluster Westerlund 1
The Galactic Super Star Cluster Westerlund 1

... Whereas we would expect ~10 -3 of the kinetic energy of winds and supernovae to be dissipated in X-rays,or ~10 36 erg s-1, the luminosity of the diffuse X-ray emission is only 6x10 34 erg s-1 (0.58.0 keV). This represents a factor of 10 deficit in diffuse X-ray emission. Moreover, the diffuse flux i ...
Comments from John Saunders.
Comments from John Saunders.

... Although when we look up at the two pointers two the Southern Cross (Alpha & Beta Centauri – Alpha being the brightest) what we don’t realise is that Alpha Centauri is actually a double or binary star. In other words, it is not one but two stars and they rotate around each others centre of gravity e ...
Learning Objectives
Learning Objectives

... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
Name: pd: ______ Date: Constellation Scavenger Hunt! Google Sky
Name: pd: ______ Date: Constellation Scavenger Hunt! Google Sky

... - Find the constellation Orion & name the stars in Orion’s Belt a) ____________________________________________ b) ____________________________________________ c) ____________________________________________ 3. If you click on the stars and read the information windows for each, you will find two of ...
The Solar System
The Solar System

... • A solar system consists of a star and objects that revolve around it. • Our Solar System consists of the Sun and nine known planets and the moons that orbit those planets. • The force of gravity keeps planets in orbit around the sun. ...
High Mass Stellar Evolution
High Mass Stellar Evolution

... If the mass of the core is > 1.4 Msolar then a neutron star is formed. If the mass of the core is > 3.0 Msolar then a black hole is formed. Important: Note that these values are for the mass of the core left over – not the initial mass of the star. Note: The 1.4 Msolar limit is known as the ...
d = 1 / p
d = 1 / p

... parallax angles). At the present the smallest parallax angle we can measure is about 0.001 arcsec, or 1000 parsecs (about 3300 light years). This is enough for most of the stars we see in the sky, but not most of the stars in the Galaxy (which is over 20000 parsecs across). Inverse Square Law – Calc ...
VARIATIONS IN SOLAR RADIATION AND THE CAUSE OF ICE AGES
VARIATIONS IN SOLAR RADIATION AND THE CAUSE OF ICE AGES

d = 1 / p
d = 1 / p

... parallax angles). At the present the smallest parallax angle we can measure is about 0.001 arcsec, or 1000 parsecs (about 3300 light years). This is enough for most of the stars we see in the sky, but not most of the stars in the Galaxy (which is over 20000 parsecs across). Inverse Square Law – Calc ...
Exam Name___________________________________
Exam Name___________________________________

... A)  A theory can never be proved beyond all doubt; we can only hope to collect more and more  evidence that might support it.  B) A theory cannot be taken seriously by scientists if it contradicts other theories developed by  scientists over the past several hundred years.  C)  If even a single new  ...
LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034
LOYOLA COLLEGE (AUTONOMOUS), CHENNAI – 600 034

... 13. Define sidereal time ‘t’ and prove that sidereal time is equal to the R.A. ± Hour angle of a star. 14. Find roughly the distance of a star whose parallax is 0.5” given that parallax of the sun is 9” and the earth’s radius is 4000 miles. 15. Prove that equation of time vanishes four times a year. ...
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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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