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Sunstruck
Sunstruck

... the core, and the dense helium core compresses the nearby layers. This causes the layers near the core to begin fusing hydrogen into helium again, but at a faster rate than before. The helium being created continues to be deposited into the core and the rate of hydrogen fusion will continue to speed ...
The Sun
The Sun

... The average solar density is approximately 1400 kg/m3, and is quite similar to that of the jovian planets and about one-quarter the average density of ...
PRE-LAB
PRE-LAB

... painted on the inside of this dome. You see the EARTH only as far as the HORIZON and to you it looks like a circular flat disk. The point directly above you (the top of the dome) is called the ZENITH. Once you locate and face the POLE STAR, you also know that that direction is NORTH. SOUTH is opposi ...
Basic Properties of Light
Basic Properties of Light

The Sun
The Sun

... Our Sun is a star, and a fairly average star at that, but with one unique feature: it is very close to us It is 300,000 times closer than our next nearest neighbor, Alpha Centauri. Alpha Centauri is 4.3 light years from us the Sun is only 8 light minutes away from us. ...
Sunspots Magnetic Field
Sunspots Magnetic Field

... sunspots, which are regions of strong magnetic field on the photosphere. Sunspot temperature is 4000 K compared to 6000 K elsewhere in the photosphere. Sunspot magnetic field is about thousand times stronger than the photosphere average. Sunspots occur in pairs, above and below the sun’s equator, an ...
introduction to astronomy
introduction to astronomy

... Compare the structure and formation of the Milky Way Galaxy with the other types of galaxies in our Universe Learning objectives What you will learn as you master the competency: a. ...
Eccentricity
Eccentricity

8hrdiagram1s
8hrdiagram1s

... Above the main sequence we have stars that are bright but cool ...
Dorn_projectF08 - Bowling Green State University
Dorn_projectF08 - Bowling Green State University

... this planet he has looked in the night sky and marveled at the ever changing appearance of its surface. The Moon orbits at roughly 380,000 km. distance with a diameter of 3475 km., compared to Earth it is 27% smaller with a reflection magnitude at opposition of -12.7. The best views through a telesc ...
My power point presentation on spectroscopy of stars (ppt file)
My power point presentation on spectroscopy of stars (ppt file)

... • This star shows strong Zeeman splitting in almost every spectral line, due to a magnetic field of 14.5 kG (1.45 Tesla) • The trace elements in the atmosphere are stratified vertically and horizontally patchy. I have not included enough of these effects in my model to reproduce the observed spectru ...
FREE Sample Here
FREE Sample Here

... demonstrating the Moon’s orbit (with fixed nodes) as you walk around your model Sun: The students will see that eclipses are possible only during two periods each year. If you then add in precession of the nodes, students can see why eclipse seasons occur slightly more often than every 6 months. The ...
Astro Midterm Review Part II: Ch 2
Astro Midterm Review Part II: Ch 2

... E) a fluorescent light ...
The Butterfly Nebula (NGC 6302)
The Butterfly Nebula (NGC 6302)

... of hydrogen fuel and reach retirement age. This is when these stars begin to stand out. As the fuel is exhausted, they first expand to enormous sizes, becoming what are called “red giants.” Then they shed their outer lay­ers into space, producing the beautiful shapes of planetary nebulae. Finally, t ...
Quantum Well Electron Gain Structures and Infrared Detector Arrays
Quantum Well Electron Gain Structures and Infrared Detector Arrays

... • Early plate tectonics brings up internal H2O and CO2 from early limestone into atmosphere • No surface water  no way of trapping CO2 , so it stays in the atmosphere now (huge pressure, greenhouse high temps) • Internal water lost  important lubricant for plate tectonics; plate tectonics stops ...
formation2
formation2

... by gravity, it fragments into smaller pockets of gas which go on to form individual stars. • The result is a star cluster. The more massive pockets from massive stars, the less massive form smaller stars, like the Sun ...
Photometry
Photometry

... For example: A player tries 10 throws in a game. On average she would make 8.5 (but obviously you can’t have a half throw!). The square root of 8.5 is 2.9 so one should expect to see a number of throws made in the range of 8.5-2.9 to 8.5+2.9 or 5.6 to 11.4 so making only 6 throws wouldn’t be so unus ...
WK7
WK7

... (rebound) Supernova events. ...
ASTRONOMY 113 Laboratory Kepler`s 3rd Law and the Mass of Sgr A
ASTRONOMY 113 Laboratory Kepler`s 3rd Law and the Mass of Sgr A

... combined – 30 billion times more powerful than our sun. It can be traced back all the way to the central object of Virgo, where it is produced in a volume about as small as Saturn’s orbit around the sun. This, finally, is the manifestation of the beast that lives within the center of M87. You have p ...
chapter 7
chapter 7

... Astronomers have now detected hundreds of planetary bodies, called exoplanets, moving in orbit around other stars. Most of these are more massive than any of the Sun's planets. These planetary-like bodies are detected because of their strong gravitationally interactions with their stars. However, te ...
Astronomy Part 2 - Malvern Troop 7
Astronomy Part 2 - Malvern Troop 7

... 5 The Planets a) List the names of the five most visible planets. Explain which ones can appear in phases similar to lunar phases and which ones cannot, and explain why. b) Find out when each of the five most visible planets that you identified in requirement 5a will be observable in the evening sk ...
HR Diagram Activity - Mr. Alster`s Science Classes
HR Diagram Activity - Mr. Alster`s Science Classes

... Purpose: In this lab we will investigate the relationship between the temperature, brightness and diameter of stars. Introduction The H-R Diagram is a tool that astronomers use to classify stars based on their luminosity, magnitude, temperature, spectral class and evolutionary stage. The H-R Diagram ...
Gravitational Forces
Gravitational Forces

... the Earth but with a radius that is 3.5 times less than the Earth’s . ___________________________________________________________________________________ ___________________________________________________________________________________ ______________________________________________________________ ...
Galaxies
Galaxies

Major Stars of the Orion Constellation
Major Stars of the Orion Constellation

... interferometer on the Mount Wilson 100 inch telescope”. [Betelgeuseweb] Recent Hubble images taken in 1995, reveal a giant “hotspot” on its disk. This bright area is some 2000 K hotter than the surrounding surface. As mentioned earlier, along with other stars in the Orion constellation, it’s thought ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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