The universe
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Transcript of The universe
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THE UNIVERSE
Trotter 2014
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IV. The Sun A. All life on Earth depends on the energy that
comes from the star in the center of our solar system.
B. Energy produced by the Sun is due to hydrogen atoms fusing together to produce helium atoms.
C. The Sun is composed of 3 layers: 1. Photosphere – innermost not as hot 2. Chromosphere – transition zone 3. Corona – largest & hottest layer
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V. Sun Surface Features A. The sun appears to
be a smooth layer but has many surface features including: 1. Sun spots – cooler
areas 2. Prominences – arching
columns of gas 3. Flares – gases
shooting straight upward 4. CMEs (coronal mass
ejections) – auroras All due to magnetic field & reactions across the Sun.
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Solar Flares
The sun unleashed a powerful solar flare late Monday (Oct. 22), releasing waves of radiation into space that have already caused a short radio blackout on
Solar flares are caused when magnetic activity ramps up in certain patches, called sunspots, on the surface of our sun
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Auroras
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Solar Eclipse
Occurs when the Sun, Moon, and Earth line up
Can only happen during a New Moon
Generally, they occur every 2-5 years
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Lunar Ecipse
Occurs during a Full Moon
Occurs when Moon, Earth, and Sun are directly aligned.
Next one is October 8, 2014
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Sun Cycle
Cycle lasts about every 11 years
Done so by counting sunspots
Sunspots may exist anywhere from a few days to a few months, but they eventually decay, and this releases magnetic flux in the solar photosphere
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I. Constellations
A. Constellations are patterns of stars that are named as a group. (88 exist in our sky)
B. All the constellations we see in the sky are part of our galaxy (large collection of stars, gas, & dust held together by gravity), the Milky Way Galaxy
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II. Absolute & Apparent Magnitude
A. The actual brightness of the star refers to the stars absolute magnitude.
B. How bright the star actually is to the viewer on Earth is called the apparent magnitude Apparent Magnitude does not equal absolute
magnitutde
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III. Measuring in Space A. Distance in space is measure in light years
or the distance light travels in one year (9.5 trillion km) Used to estimate the distance of stars from Earth The distance shifts depending on the
motion/position of Earth as it orbits (parallax)
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Astronomical Unit: the distance between the Earth and the Sun
149 597 871 kilometers
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VI. Properties of Stars
A. Basic properties of stars include: 1. Diameter 2. Mass 3. Brightness 4. Energy Output (luminosity) 5. Composition – 73% hydrogen, 25% helium 6. Surface Temperature – appears different due to
very slight composition differences
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VII. Classifying Stars A. Hertzsprung & Russell Diagram shows the
relationship of temperature & brightness among stars
B. Main Sequence(90%) vs. Dwarfs & Giants (bright)
Temperature: x axis Absolute Magnitude: y axis
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IIX. Life of a Star Scientists theorize that a star goes through a
few steps (as hydrogen depletes) 1. Nebula – ball of gas & dust 2. Main sequence – pieces of nebula are pulled
together due to gravity, force increases energy/temperature
3. Red Giant vs. Red Super Giant – when hydrogen begins to deplete outer layer cools & expands, (if large sequence is more quick & violent)
4. White Dwarf vs. Neutron Star or Black hole – outer layers cool & escape to space leaving hot dense core
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Star Vocab
Binary star Parallax H-R Diagram Stellar nebula Massive star Red supergiant Red giant Planetary nebula Supernova White dwarf Neutron star Black hole Absolute magnitude Apparent magnitude
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Classwork Activity
Star Cycle Flip Book or Comic Strip Must include all aspects of the star cycle For each step, there must be accurate
vocabulary and a small narrative describing what happens
Students will be graded on vocabulary, narratives and aesthetics
This should be turned in by the end of the week in order to remain on track (2/22/2014)
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We are now here
Life cycle of our sun
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They discovered that stars grouped by type and during their lifetimes would move from one place on the graph to another. As our sun ages, it will move to a giant star to a white dwarf.
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IX. Galaxies
A. Galaxies are groups into clusters. B. Types of galaxies:
1. Spiral Galaxies 2. Elliptical Galaxies – football 3. Irregular Galaxies – small irregular
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X. Gravitational Pull
A. Every 2 bodies in the universe attract each other with a force that is proportional to the product of their masses.
In other words gravitational force depends on their masses & the distance between the 2 bodies
Gravity increase with larger mass & closer proximityThink about 2 magnets