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Our galaxy, the Milky Way, has about 3 billion solar masses of HI
Our galaxy, the Milky Way, has about 3 billion solar masses of HI

... their distance by some means such as stellar parallax or some other method. Once the luminosity a these stars are measured (by comparing their apparent magnitudes and their distance) and once the luminosity is established as constant for all objects of that class, then the luminosity of one of these ...
Origin of Our Solar System
Origin of Our Solar System

... Nebular Hypothesis In 1755 Immanuel Kant proposed that a solar nebulae was pulled together by gravity so that it collapsed into a flat, rotating disk that eventually coalesced into the Sun and planets ...
Robotics - UNL CSE
Robotics - UNL CSE

... exploration of space and the search for extra-terrestrial intelligence is driven by the power of computers and computer science. Without computers, there would be no rovers, no computer models of other planets, no high-powered telescope and satellite arrays to scan the frequencies for communications ...
PROBLEM SET #9 SOLUTIONS AST142 1. Quasar luminosity
PROBLEM SET #9 SOLUTIONS AST142 1. Quasar luminosity

... is accreting at the Eddington rate, and show that these two findings are consistent with one another. ...
Solar System 2010 - Science Olympiad
Solar System 2010 - Science Olympiad

... The nucleus is a few kilometers across and is surrounded by a diffuse, bright region called the coma that may be a million kilometers in diameter.The coma is formed from gas and dust ejected from the nucleus as it is heated by the Sun. The coma is bright both because it reflects sunlight and becau ...
N (North) Equator Latitude and Declination
N (North) Equator Latitude and Declination

... The observed altitude of a star is its angular distance above the observer’s horizon. A star’s altitude will vary with the time of observation. A star’s declination is its angular distance above the celestial equator. The declination is also 90 degrees minus the angle the star makes with the earth’s ...
Solar System 2010 - Science Olympiad
Solar System 2010 - Science Olympiad

G W ORIONIS, A 20000 YEARS OLD T TAURI STAR? 1\/"", _ 0.14
G W ORIONIS, A 20000 YEARS OLD T TAURI STAR? 1\/"", _ 0.14

... Our knowledge 01' the actual ages 01' very young stars is very meager; the first indication Lhat we may be observing stars with ages 01' the onler 01' 10 000 years came indirectly from the analysis 01' the density distribution in the Orion nebula (Kahn am! Menon ]9(1) which showed that the latter co ...
Bad Astronomy - Eastbay Astronomical Society
Bad Astronomy - Eastbay Astronomical Society

The Motion of Celestial Bodies
The Motion of Celestial Bodies

Secrets of the Sun
Secrets of the Sun

... Seasonal patterns of sunrise and sunset can be observed, described, and predicted. (By end of grade 2). The orbits of Earth around the sun and of the moon around Earth, together with the rotation of Earth about an axis between its North and South poles, cause observable patterns. These include day a ...
Lecture 16
Lecture 16

... A. In this system the lower mass star must have evolved faster than the higher mass one. B. The red giant might be made of some different elements, so it evolved faster. C. The lower mass star used to be a more massive main sequence star, but when it became a giant some of its mass went onto the oth ...
THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting
THE GALACTIC GAZETTE The Astronomical Society of Southern New England Next Meeting

... layers respond by inflating hugely, like a hot air balloon. The heat from the interior gets spread out through the much ...
A Collection of Curricula for the STARLAB Deep Sky Objects
A Collection of Curricula for the STARLAB Deep Sky Objects

... Nebulae absorb light from nearby stars and radiate it back into space. Most nebulae glow red, the color of hydrogen gas. The brightest nebula is the Orion Nebula (see slide #60) which can be seen with the unaided eye in a dark sky. Nebulae are very important in astronomy because they are the key to ...
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... condense to form solids. C,N,O are the most common elements after H,He ...
The Ring Nebula, NGC 6720
The Ring Nebula, NGC 6720

... The Ring Nebula (NGC 6720) is a bright, glowing gas cloud that is a favorite of both amateur and professional astronomers alike. Located in the constellation Lyra (the lyre, or harp), the nebula is situated within the famous Summer Triangle of bright stars (Vega, Altair, and Deneb) for northern hemi ...
16 October 2006
16 October 2006

... they form, because it is a noble gas. • Therefore the ratio of argon-40 to potassium-40 is a direct measure of a rock’s age. • Possible problem: Heating a rock can allow trapped argon atoms to escape. If a rock has been heated, it might be older than we think it is. ...
exo planets
exo planets

... star. The planet may have the potential for life to exist. The world circles a red dwarf star in the constellation of Cygnus and is about 500 light years away. The planet is known as Kepler 186f and is about 10% larger than the Earth. It is the outermost planets in the 186 system and takes 130 days ...
Formation of the Solar System
Formation of the Solar System

... opposite way were likely captured. Most of these moon are small are lie far away from the planet. • Giant impacts – may have helped form the Moon and explain the high density of Mercury and the Pluto-Charon system. Furthermore, the unusual tilts of Uranus and Venus can also be explained by giant imp ...
Supernova - Mid-Pacific Institute
Supernova - Mid-Pacific Institute

... supported by the release of nuclear energy.  If the star is particularly massive, then its core will collapse and in so doing will release a huge amount of energy. This will cause a blast wave that ejects the star's envelope into interstellar space. ...
Sky, Celestial Sphere and Constellations
Sky, Celestial Sphere and Constellations

Piscataway High School - Piscataway Township Schools
Piscataway High School - Piscataway Township Schools

... Identify Scientists who made a contribution to Modern Astronomy Explain ellipse geometry and eccentricity of planetary orbits Apply Kepler’s three Laws of Planetary Motion Name the major regions and differences between parts of the electromagnetic spectrum Explain how reflecting and refracting, radi ...
SUMMARY White dwarfs, neutron stars, and black holes are the
SUMMARY White dwarfs, neutron stars, and black holes are the

... in an accretion disk. What type of photons have this wavelength? 10. (15.1–15.3) You observe a main sequence K0­type star that moves as if it is in a binary system, but no companion is visible. If the period of the system is 34 days and the semimajor axis is 0.5 AU, what is the mass of the system (r ...
Ans. - Testlabz.com
Ans. - Testlabz.com

... Q.40. Does the sun rise in east and set in west on Venus? Ans. Yes, the sun rises in the east and sets in the west on Venus as rotation of Venus on its axis is from east to west. ...
5 Sun`s Motion
5 Sun`s Motion

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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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