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Profile Documents Logout
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Word doc - UC
Word doc - UC

Universe Notes - Solon City Schools
Universe Notes - Solon City Schools

... What force is responsible for causing interstellar material to condense and form our sun? GRAVITY ...
25 August: Getting Oriented, Astronomical Coordinate Systems
25 August: Getting Oriented, Astronomical Coordinate Systems

Multiple choice test questions 1, Winter Semester
Multiple choice test questions 1, Winter Semester

... C) It appears very near the north celestial pole. D) It is the star directly on your northern horizon. E) It can be used to determine your longitude on Earth. 10) Which of the following never goes in retrograde motion? A) the Sun B) Venus C) Mars D) Jupiter E) Saturn 11) Which planet is moving most ...
Ages of Star Clusters - Indiana University Astronomy
Ages of Star Clusters - Indiana University Astronomy

The Hidden Lives of Galaxies NSTA 2001
The Hidden Lives of Galaxies NSTA 2001

... How I Wonder What You Are ... Stars have • Different colors  Which indicate different temperatures ...
good - Cosmos
good - Cosmos

Place in Space
Place in Space

... Q2: A galaxy is a system of stars, dust, and gas held together by gravity. Our solar system is in a galaxy called the Milky Way. Astronomers have photographed millions of galaxies through telescopes. The most distant galaxies ever photographed are as far as 10 billion to 13 billion light-years away. ...
Replace this sentence with the title of your abstract
Replace this sentence with the title of your abstract

Introduction to Astronomy - Northumberland Astronomical Society
Introduction to Astronomy - Northumberland Astronomical Society

... We’ll also examine how our location on the Earth affects the stars and constellations we can see and how changes in the tilt of the Earth’s axis change the view over long time periods. ...
Star - Danielle`s science9 weebly
Star - Danielle`s science9 weebly

... of reference being the Earth. To track the actual motion of each celestial body in space, you need to use the stars as your frame of reference, instead of the Earth. To do this you would make an observation of which celestial body you are studying and include other stars in relation to it. Make subs ...
PPT
PPT

...  90% of life cycle as a main sequence  fusing Hydrogen into Helium  **always present is the “equilibrium” ...
Measuring the ligth
Measuring the ligth

... of 10 pc, one pc (parsec or second of parallax) is the distance at which one astronomical unit subtends and arc of one arc second and is more or less 3.26 light years. The absolute magnitude is related to the luminosity and it’s easy to prove knowing the Suns absolute magnitude and luminosity Mo and ...
Section 25.2 Stellar Evolution
Section 25.2 Stellar Evolution

...  Massive stars use fuel faster and exist for only a few million years.  Small stars use fuel slowly and exist for perhaps hundreds of billions of years.  A star spends 90 percent of its life in the main-sequence stage. Red-Giant Stage  Hydrogen burning migrates outward. The star’s outer envelope ...
Lecture 13
Lecture 13

... To say you were 5mph over the limit needs to measure one part in 100million! ...
Module 6: “The Message of Starlight Assignment 9: Parallax, stellar
Module 6: “The Message of Starlight Assignment 9: Parallax, stellar

... light years. (A light year is how far light travels in a year.) Now, if we know the distance to the star, we can convert its brightness, measured in magnitudes (mag), to the magnitude a star would have at a fixed distance which has been chosen to be 10 parsecs, or about 32.6 light years. The equatio ...
Weathering, Erosion and Mass Movement
Weathering, Erosion and Mass Movement

... violent eruptions from the Sun’s surface called solar flares. ...
The Life of a Star
The Life of a Star

... 2. Describe the differences between the life of a low-mass star and that of a star 10 times the Sun’s mass. Low-mass stars cool down and swell up into a red giant. Outer layers drift away and the star shrinks to become a white dwarf which will cool and fade away. High-mass stars swells into a red su ...
CASPEC Observations of the Most Metal-Deficient Main
CASPEC Observations of the Most Metal-Deficient Main

... shown for this star and a sequence of stars with decreasing values of [MgIH]. The stars are main-sequence turnoff stars and have about the same effective temperature as CS 22876-32 (Teff = 6000 K) according to the Strijmgren uvby-(3 photometry. The remarkable line weakness of CS 22876-32 is obvious ...
File
File

File - Awakening in Grade 6
File - Awakening in Grade 6

... Earth, our Sun appears to trace a circular path. This path defines a plane called the plane of the ecliptic (or just the ecliptic). The zodiac is the group (or “belt”) of constellations that fall along the plane of the ecliptic. It is through these constellations that our Sun appears to “pass” durin ...
Measuring the Properties of Stars (ch. 17)
Measuring the Properties of Stars (ch. 17)

... you the temperature, so you can just read off the luminosity from the H-R diagram. Knowing the apparent brightness (really easy to measure) and luminosity, this gives the distance (review earlier material if you don’t understand this), without having to get a trigonometric parallax. Distances obtain ...
Binocular Universe: Bikini Bottom
Binocular Universe: Bikini Bottom

... The second double star is Dabih, or Beta (β) Capricorni, is just south of Algedi in the same field of view. While Algedi's two stars appear identically bright, Dabih's two stars look markedly different. The brighter sun, called Dabih-Major, shines at 3rd magnitude, while its companion, Dabih-Minor, ...
Stellar Classification and Evolution What is a star? A cloud of gas
Stellar Classification and Evolution What is a star? A cloud of gas

Directed Reading A
Directed Reading A

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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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