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Space environment
Space environment

Today`s Powerpoint
Today`s Powerpoint

... weightless. Einstein says these are equivalent. So in freefall, the light and the ball also travel in straight lines. 3. Now imagine two people in freefall on Earth, passing a ball back and forth. From their perspective, they pass the ball in a straight line. From a stationary perspective, the ball ...
Night/Day and Earth Years
Night/Day and Earth Years

Star Maps and Constellations (pdf 3.7 Megs)
Star Maps and Constellations (pdf 3.7 Megs)

... magnitude, so numbers "less" than 1 have to be used. For example, Vega has a magnitude of 0, meaning it is brighter than a first magnitude star. The brightest star is Sirius, with a magnitude of 1.5, even brighter than Vega. The moon on this scale is -12.5, the sun -26.8 (see Table SC-VI). Polaris w ...
solar cycle
solar cycle

... conversion in the Sun called nuclear fusion was found: – Sun’s core temperature is high enough to force positively charged protons close enough together to bind them together via the nuclear or strong force – The net effect is that four protons are converted into a helium nucleus (plus other particl ...
Chapter 11
Chapter 11

... conversion in the Sun called nuclear fusion was found: – Sun’s core temperature is high enough to force positively charged protons close enough together to bind them together via the nuclear or strong force – The net effect is that four protons are converted into a helium nucleus (plus other particl ...
Planets
Planets

...  Both Uranus and Neptune do contain a significant hydrogen and helium atmosphere, but they are dominated by ices in liquid form ...
Olbers` Paradox - NMSU Astronomy
Olbers` Paradox - NMSU Astronomy

... the line of sight argument: In an infinite, homogeneous Universe every line of sight will end upon the surface of a Star. So why is the sky dark at night? The advantage offered by this argument is that it doesn’t require the stars to be randomly scattered in space, but also works if the stars are g ...
Small Bodies of the Solar System Transcript
Small Bodies of the Solar System Transcript

... in diameter; Vesta 525 km and Pallas 540 km and Juno 230 km; and decrease in size down to rocks barely tens of metres in diameter. As with so many natural distributions, there are fewer of the larger objects, and ever-increasing numbers at progressively smaller sizes. We expect that there are over ...
Kuiper Belt
Kuiper Belt

... Dwarf Planets • Among lots of smaller debris, which we’ll discuss in a few moments, Pluto is joined by a few other dwarf planets, a term I first used last lesson. – Dwarf planets are essentially very large asteroids – also a term we’ll get to – but don’t quite meet the requirements of being a plane ...
The magnitudes of stars
The magnitudes of stars

... However this does not give a true impression of the actual brightness of a star. A nearby faint star may well look brighter than another star that is actually brighter but more distant. (A good example of this is shown by Rigel and Sirius in the following table. Sirius looks brighter than Rigel when ...
Dear Teachers - Jeffrey Bennett
Dear Teachers - Jeffrey Bennett

... Scale Activity 2: The Solar System Before you begin: • Find a ball or piece of fruit (grapefruits work well) approximately 14 cm in diameter, to represent the Sun. • (optional) You can use clay or a set of ball bearings to use as models for the planets. • You will need a ruler and tape measure. • Y ...
Powerpoint for today
Powerpoint for today

... weightless. Einstein says these are equivalent. So in freefall, the light and the ball also travel in straight lines. 3. Now imagine two people in freefall on Earth, passing a ball back and forth. From their perspective, they pass the ball in a straight line. From a stationary perspective, the ball ...
Lecture 3 - The University Centre in Svalbard
Lecture 3 - The University Centre in Svalbard

... The Moon orbits the Earth, which in turn orbits the Sun. Thus, sometimes the Moon will be located between the Earth and the Sun and we will experience what we call a solar eclipse. By a coincidence he Sun and the Moon appear to have the same size in the sky as seen from the Earth. The shadow of the ...
Measuring Distances: Mph (miles per hour): miles traveled per hour
Measuring Distances: Mph (miles per hour): miles traveled per hour

... Theories  can  change  if  EVIDENCE  supports  the  change.  Theories  about  the  origins  of  the  universe   include:    Flat  Earth  Theory,  Ptolemy  Universe  Theory,  Copernicus  Universe  Theory,  Kepler’s  Universe   Theory,  Steady ...
ppt
ppt

... as silicates and metals can condense to form solids At larger distances ices (both water and ammonia) can condense due to the lower temperatures ...
Light Years - Spring Creek Elementary
Light Years - Spring Creek Elementary

... 7,440,000,000 miles, 80 AU, or about .00127 light years. That actually makes it sound small! The closest star to our Solar System is Proxima Centauri in the Alpha Centauri star system, which is about 4.4 light years away. The largest star within ten light years is Sirius. It is about 8.6 light year ...
Starry Night¨ Times - October 2008
Starry Night¨ Times - October 2008

... At Mag -1.5, almost everyone knows that Sirius is the brightest star in the night sky. You may notice it driving home from work: visible from early dusk, it sparkles brilliantly above the southern horizon. What many people don't realize is that Sirius is actually a double star. Sirius B is a challen ...
R E P O R T 5 - WordPress.com
R E P O R T 5 - WordPress.com

... The Archean is the name of the age which began with the forming Earth. Following the Hadean Eon and preceding the Proterozoic Eon. During the Archean, the earth's crust and layers had just formed, making the Earth much cooler than it was during the Hadean and allowing the formation of continents. ...
Astronomy Final C - Tarleton State University
Astronomy Final C - Tarleton State University

... 17. During the Radiation Era A.the Universe was too hot for atoms to be stable B.the Universe had cooled enough where atoms could be stable 18. ? Geometry is “closed” geometry. A.Euclidean B.Spherical C.Hyperbolic D.all of these are “closed” geometries 19. Which of the following astronomical bodies ...
Basic Patterns and Motions in the Sky
Basic Patterns and Motions in the Sky

...  Above: + (you can see it)  Middle: 0º (The horizon itself)  Below: – (you can’t see it) o Azimuth – Angle around the celestial sphere:  North: 0º/360º azimuth  East: 90º azimuth  South: 180º azimuth  West: 270º azimuth  These 4 direction can be labeled on the horizon as North, East, South, ...
AST 341 Final Exam and Solutions
AST 341 Final Exam and Solutions

... (b) The binding energy of Fe56 is about 9 MeV per nucleon; that of He4 is about 7 MeV per nucleon. If the main sequence lifetime of a 50 M⊙ star is about 5×106 years, what is its average luminosity while on the main sequence? Proceed as in problem 1. 10% of the stellar mass is in the core. This is 5 ...
Midterm Exam, AST 203, Spring 2012 Thursday, March 15, 3:00
Midterm Exam, AST 203, Spring 2012 Thursday, March 15, 3:00

... • He saw that Venus went through phases, easily explained (and predicted!) in the heliocentric view, and not expected in the geocentric view. (3 points) • He saw that Jupiter had a set of four moons orbiting around it, showing directly that heavenly bodies can exhibit circular motions around objects ...
HW7-3
HW7-3

... (260) RQ 3: What is a brown dwarf? A brown dwarf is a “failed star.” They are balls of gas without fusion. The upper end of brown dwarfs is well defined: 8% M☉ = 80 Jupiters. There is a not-so-welldefined line between small brown dwarfs and large planets. (260) RQ 6: Why do expanding stars become co ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... (The Leviathan of Parsonstown shown, 1845 Biggest telescope of the World until 1917) ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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