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Scaling the Solar System
Scaling the Solar System

... actual diameter by the scaling factor. Likewise, to find the model distance from the sun divide the actual distance by the scaling factor. Be sure to use proper units in your example calculations since you want students to have an understanding of the units as well. 10) Assign one planet to each pai ...
Which Constellation is Which?
Which Constellation is Which?

... The stars look like they are all the same distance away. That’s not true. The stars in the sky are different distances from Earth. ...
THE EARTH AND MOON
THE EARTH AND MOON

Astronomy
Astronomy

Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

... – Very common systems; currently estimated to be even more common than single stars in our Galaxy. – Useful in estimating stellar masses: mass can be calculated when the orbital period is known (as stated by Kepler’s III ...
Power Point Presentation
Power Point Presentation

... Its atmosphere is very hot (1100oC) since it is only 6.4 million km from the star When the planet passed in front of the star, the star’s light passed through the planet’s atmosphere and sodium was observed by HST ...
Cosmos & Contact - Access Research Network
Cosmos & Contact - Access Research Network

... the star system Vega. • The signal is seen to be more than radio noise by the presence of prime numbers, indicating an intelligent source. ...
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... It provides a way of measuring the number of civilizations in the galaxy. If the equation comes out with a low number, than the reason that we haven’t found/heard from aliens is that there aren’t any…if the number is high, the ...
The Death of Stars
The Death of Stars

... • Supernovae produce remnants: expanding shells of gas rich with heavy elements. • Perhaps the most famous is the “Crab Nebula” from a supernova in 1054 AD. It was so bright, Chinese, Japanese, and Arab astronomers saw it for months during the day, and could be seen for 2 years at night. • The remna ...
Dark Matter Dark Energy The History of the Universe More of the
Dark Matter Dark Energy The History of the Universe More of the

Astronomy 82 - Problem Set #1
Astronomy 82 - Problem Set #1

... . Since we already found ac, this immediately ac gives the planet's orbital velocity amplitude: 20 km/s. We can now return to our initial equation to solve for the final quantity we desire. v* ...
Unpublished draft available in  format
Unpublished draft available in format

... groups (the most comprehensive unit of aggregation), galaxies, sub-galactic systems, starsystems, etc. Provision for the general treatment of any notional body or system (from particles, through dust to planets, stars and galaxies) is theoretically necessary (e.g. the general idea of a satellite bod ...
STAR MAKER Olaf Stapledon
STAR MAKER Olaf Stapledon

... the nether constellations. The two domes of the sky were fused into one hollow sphere, star-peopled, black, even beside the blinding sun. The young moon was a curve of incandescent wire. The completed hoop of the Milky Way encircled the universe. In a strange vertigo, I looked for reassurance at th ...
presentation source
presentation source

... The Stars and their Environment ...
Stellar Evolution Hertzsprung-Russell Diagram Hertzsprung
Stellar Evolution Hertzsprung-Russell Diagram Hertzsprung

... some go through nova/supernova stage most become black dwarfs and disappear ...
Comets, Meteors, and Meteoroids
Comets, Meteors, and Meteoroids

... The dust comes from comets. These pieces of comet dust are called meteoroids. Most meteoroids are smaller than a grain of sand. The flash of light is called a meteor. Meteors usually last just a second or two. Sometimes, there are meteor showers. In a meteor shower, lots of shooting stars seem to fa ...
Workbook IAC
Workbook IAC

... months. Comets appear to be bright balls with fat tails. They do not fall rapidly in the sky; you would have to watch one for hours or days to see its movement. The center of a comet is a ball of frozen gas, dust, and water. Like planets or moons, comets orbit around the Sun. The comet that causes ...
Star Life Cycle Powerpoin
Star Life Cycle Powerpoin

... sequence star is consumed, fusion stops and the forces suddenly become unbalanced. Mass and gravity cause the remaining gas to collapse on the core. ...
Life Cycle of a Star
Life Cycle of a Star

... Nuclear fusion is the engine of the star. Hydrogen will convert to helium at the rate it takes to support the stars mass. For bigger stars, nuclear fusion must occur at a very fast rate in order to balance the star’s gravity. Because of this, larger stars go through the stages much faster than small ...
Maya .(English)
Maya .(English)

... Moon’s orbit is 27.322days Moon marker – twice a day and skip one each cycle ...
Document
Document

... “Another is the study of the center of our galaxy, where a black hole with four million times the mass of the Sun resides,” De Zeeuw relates. “Observations of this region with the new GRAVITY instrument on the VLT are starting to test Einstein’s general theory of relativity in much stronger gravity ...
The 22 First Magnitude Stars
The 22 First Magnitude Stars

Word
Word

... #3. The giant elliptical galaxy M87 has an accretion disk of material orbiting its central black hole. The Hubble Space Telescope observed the spectrum of this material and, from the Doppler shifts of the spectral lines, found that the material is orbiting at 550 km/sec at a distance of 40 pc from t ...
HOMEWORK #1
HOMEWORK #1

... #3. The giant elliptical galaxy M87 has an accretion disk of material orbiting its central black hole. The Hubble Space Telescope observed the spectrum of this material and, from the Doppler shifts of the spectral lines, found that the material is orbiting at 550 km/sec at a distance of 40 pc from t ...
Atmospheric Composition
Atmospheric Composition

... Mass of Earth’s atmosphere Mass = 4 π R2 P(surface)/ g ≈ 5 × 1018 kg. (1 kg / cm2). This is the same weight as a column of water 10 meters deep. Air is 78% N2, 21 % O2, and 1% Ar (+ some water and other things). The mean molecular weight, Ma, is: (0.78 × 28) + (0.21 × 32) + (0.01 × 40) = 29 g mole-1 ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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