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View slides as PowerPoint
View slides as PowerPoint

... • Above atmospheric turbulence, should achieve contrast performance better than ground AO and approaching that of a space platform • Operate at visible wavelengths with 1-m telescope, deploy coronagraph with precision wavefront control • Small telescope can still be very sensitive to extended surfac ...
Chapter-6 Lecture Spring Semester
Chapter-6 Lecture Spring Semester

... 6.1 An Inventory of the Solar System More than 3,472 extrasolar planets have been found Understanding planetary formation in our own solar system helps understand its formation as well as formation of other systems Comparative planetology – comparing and contrasting the properties of the diverse wo ...
Stellar Evolution
Stellar Evolution

... • all the stars are at about the same distance from the Earth • all the stars formed at about the same time Determining the distance and age to a globular cluster is much easier than trying to find the distances and ages of a million random stars! Laboratories for understanding how stars of differen ...
Define the following terms in the space provided
Define the following terms in the space provided

... Their diameters are measured in light years. Galaxies are very large aggregations of stars, gas and dust. Our Milky Way galaxy is about 100,000 light years in diameter. Galaxies tend to be grouped in clusters that may have only a few member galaxies up to ten’s of thousands of galaxies. Our small ga ...
r*=13.6 km MPA1 EOS
r*=13.6 km MPA1 EOS

... stars known as Westerlund 1. This cluster contains a hundred thousand or more stars in a region only 30 light years across, which suggests that all the stars were born in a single episode of star formation. Based on optical properties such as brightness and color some of the normal stars in the clus ...
1-Syllabus-Intro
1-Syllabus-Intro

A Faint Star Orbiting the Big Dipper’s Alcor Discovered
A Faint Star Orbiting the Big Dipper’s Alcor Discovered

... He published details of his first observations in 1610. The book immediately made Galileo famous. It was titled Sidereus Nuncius – The Sidereal (or Starry) Messenger. In it he describes (among other things) observations of the moon, and the discovery of the four brightest moons of Jupiter. Even toda ...
How Stars Work: Ay 122 - Fall 2004 - Lecture 7
How Stars Work: Ay 122 - Fall 2004 - Lecture 7

... Sun is obviously not collapsing / exploding on this time scale! Implies that pressure and gravitational forces are in very close balance†within the Sun, i.e. Sun is very nearly static. Slow changes due to: • Changing composition (time scales of Gyr) • Mass loss due to Solar wind (even longer at curr ...
Joining the Party - Lincoln-Sudbury Regional High School
Joining the Party - Lincoln-Sudbury Regional High School

... Too bright! ...
Scientific American`s Ask the Experts
Scientific American`s Ask the Experts

... craft to encounter an asteroid while it was passing through the asteroid belt on its way to Jupiter. But it took some effort to find an object that was located even roughly along Galileo’s path. Special targeting was required to reach this object, but the result was the first close-up view of an aster ...
Cosmic Dawn A Hunting for the First Stars in the Universe
Cosmic Dawn A Hunting for the First Stars in the Universe

... the resulting heat of compression. Otherwise, restorative gas pressure will halt gravitational collapse well before the gas can reach the temperatures and densities required to sustain nuclear fusion. No stars could ever be born in this scenario. Fortunately, there are ways around the problem via mo ...
Constituents of the Milky Way
Constituents of the Milky Way

Origin of stars
Origin of stars

... will expand NOT contract ...
Part 2 of Our Lecture
Part 2 of Our Lecture

... WTTS (green) CTTS (red) HD 206267 (blue) in Tr37 High- and intermediate-mass stars (open stars) ...
Astrobiological Stoichiometry
Astrobiological Stoichiometry

... even for the stars, which are much brighter and easier to observe. The high-resolution spectra that are needed are burdensome to obtain, and for many nearby stars only the abundances of Fe, or at most a few elements, are determined. The measurement is fraught with uncertainty, often from unrecognize ...
All About Astronomy The Planets
All About Astronomy The Planets

... and others. The sun is the center of our solar system; the planets, their moons, a belt of asteroids, comets, and other rocks and gas orbit the sun. The eight planets that orbit the sun are (in order from the sun): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. Another large body is ...
Twinkle Twinkle Little Star
Twinkle Twinkle Little Star

... learning about the life cycle of stars. If you notice, the song even states that the composer doesn’t know anything about stars: “How I wonder what you are.” Directions: Now that you know about stars, your lab is to rewrite the song with accurate information. You will work in groups of three. Your s ...
Star Finder
Star Finder

... constellation?_____________________ HINT: The Sun goes from below the equator to above the equator.! Hence the FALL or AUTUMNAL EQUINOX the first day of autumn occurs when the sun is in the constellation? __________________________ The Sun is dropping below the equator. As an aside; the ancient civi ...
Falling Stars
Falling Stars

Gravitational redshifts
Gravitational redshifts

... Towards the science case for E-ELT HIRES, Cambridge UK, September 2012 ...
October - Sonoma County Astronomical Society
October - Sonoma County Astronomical Society

... Will Earth Survive? (from Page 1) ...
The amazing lives of two stars
The amazing lives of two stars

... the hyper-productive, super-brilliant orb of energy. From its early formation from an interstellar cloud, to its twilight as a white dwarf, the Sun will experience numerous phases -- the most stable of which, we're enjoying now. But what goes on inside that big, bright ball during its unstable phase ...
Chapter 17 Star Stuff How does a star`s mass affect nuclear fusion
Chapter 17 Star Stuff How does a star`s mass affect nuclear fusion

Chapter 17 Star Stuff
Chapter 17 Star Stuff

... • High-mass stars with >8MSun have short lives, eventually becoming hot enough to make iron, and end in supernova explosions • Low-mass stars with <2MSun have long lives, never become hot enough to fuse carbon nuclei, and end as white dwarfs • Intermediate mass stars can make elements heavier than c ...
2. A giant hand took one of the planets discovered
2. A giant hand took one of the planets discovered

... 2. A giant hand took one of the planets discovered around other stars and put it in the solar system at the same distance from the sun as from its star. The mass of the planet is approximately that of Jupiter and the orbit is approximately that of Earth. These are the “hot Jupiters”, as big as Jupit ...
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