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ASTRONOMY Astron – “star” nemein – “to name” ASTRONOMY Longman Dictionary of Contemporary English, 1993 astro‐ concerning the stars, the planets, or space. astronomy the scientific study of the sun, moon, stars, etc. astrophysics the scientific study of the chemical nature of the stars and the natural forces that influence them. astrology the art of understanding the supposed influence of the sun, moon, stars and planets on events and on people’s character The Scientific Method requires that our ideas about nature are consistent with what we actually observe! Assumptions: ‐ Laws of Nature are “universal” ‐ apply anywhere, at any time ‐ Nature works in simple ways Step 1: Collect Scientific Data: ‐ making observations, measurements Step 2: Form a Hypothesis: ‐ an idea or collection of ideas to explain the data ‐ must be based on scientific data ‐ must explain data completely ‐ no conflicts with any known results ‐ must be testable ‐ able to make verifiable predictions ‐ able to be proven false

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Page 1: Astron – “star” nemein – “to name”...‐ Dwarf planets (like Pluto) ‐ smaller round objects ‐ orbit near similar objects, in a “belt” ‐ Satellites (moons) of

ASTRONOMY Astron – “star” nemein – “to name”

ASTRONOMY Longman Dictionary of Contemporary English, 1993 

astro‐ concerning the stars, the planets, or    space.  astronomy – the scientific study of the sun,    moon, stars, etc.  astrophysics – the scientific study of the   chemical nature of the stars and the 

natural forces that influence them.  

astrology – the art of understanding the   supposed influence of the sun, moon,    stars and planets on events and on    people’s  character  

 

The Scientific Method requires that our ideas about nature are consistent with what we actually observe! 

Assumptions: ‐ Laws of Nature are “universal” 

‐ apply anywhere, at any time   ‐ Nature works in simple ways 

Step 1: Collect Scientific Data: ‐ making observations, measurements 

Step 2: Form a Hypothesis:   ‐ an idea or collection of ideas to  

explain the data ‐ must be based on scientific data ‐ must explain data completely 

‐ no conflicts with any known results ‐ must be testable 

‐ able to make verifiable predictions ‐ able to be proven false 

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Step 3: Test the Hypothesis   ‐ perform experiments to test     predictions, measure new data 

If the hypothesis is supported: 

 becomes widely accepted 

        Scientific Theory   If the hypothesis is not supported: 

   hypothesis has to be changed or        rejected! 

Science is a never ending process:   Scientific Theories and Models 

‐are ALWAYS open to questioning and testing!  

 A Scientific Fact:   ‐ an objective and reliable observation 

A Scientific Law: ‐ a concise statement/formula to explain    an  action or a relationship.   ‐ “rules of the game” ‐ does not explain “why” ‐ usually one part of a larger theory 

A Scientific Theory: ‐ a tested explanation based on a wide  

body of knowledge. ‐ represents the most complete  

understanding we have for any topic.  Common usage of “theory” is WRONG! 

“It’s only a theory” X   an untested idea X   an idea not based on facts X   a (wild or crazy) guess 

  

Science is NOT: ‐ a collection of bits of information 

  ‐Data is only one part of a process 

‐ Something that only can be done by highly    trained individuals 

  ‐Science is a method or way of 

   thinking 

‐ Absolute Proof   ‐Science cannot “prove” something 

 without testing every possibility     ‐Scientific evidence can only support  

a hypothesis, not prove it   ‐But, a theory can always be  

    disproven 

‐ Popular opinion  ‐ opinions won’t affect how nature  

works  

 

 

 

 

 

 

 

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Large Scale Structure of the Universe 

The size of a person is used as a reference 

 

     GPC Clarkston Campus, Google Earth 

 

 

Earth (planet) 

An object composed of liquid & solid material - may also contain some gases  - has enough gravity to become round - relatively isolated in space 

 http://apod.nasa.gov/apod/ap130331.html 

http://messenger.jhuapl.edu/the_mission/flyby_movie.html 

        The Solar System 

A system of astronomical objects including: - Earth (a planet) - Seven other planets  

Mercury Venus Earth Mars 

Jupiter Saturn Uranus 

Neptune 

 

  

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- The planets orbit around the Sun 

The SUN (a typical star) 

 http://sohowww.nascom.nasa.gov/  http://www.nasa.gov/mission_pages/sdo/main/index.html 

 

The Sun ‐contains 99.86 % of mass of solar system ‐hot ionized gas, produces energy 

Other objects in the Solar System: 

‐ Dwarf planets (like Pluto)   ‐ smaller round objects  

‐ orbit near similar objects, in a “belt”  

‐ Satellites (moons) of the planets   ‐ can be larger than a “planet”   ‐ but, if it orbits another planet  

=> “moon” 

 

 

‐ Asteroids ‐ small, irregular shape, rocky & metallic 

‐ Comets     ‐ small, icy, often with long tails 

    

Measuring Distances: - Standard units (km or miles)  

- too small, inconvenient to use - Astronomical Units (AU)  

- 1 AU = distance from Earth to Sun  (93,000,000 miles or 150,000,000 km) 

‐ Light Travel Time   ‐ uses speed of light (c) to measure      distance 

    (c = 186,000 miles/s or 300,000 km/s) 

  

1 light second = the distance light travels              in 1 second  (300,000 km) 

1 light minute = the distance light travels in            1 min.  

1 light hour = the distance light travels in  1 hr.           

Examples: Earth Circumference   = 24,900 mi; 40,000 km 

        = 0.13 light sec.   

Earth‐Moon    = 239,000 mi; 384,000 km = 1.3 light sec.   

Earth‐Sun   = 93,000,000 mi; 150,000,000 km = 8.3 light min.   

Sun‐Pluto = 3,674,500,000 mi; 5,913,500,000 km    = 5.5 light hrs  

What is “NOW”? - “Now” is when the light reaches us - No way to know anything before its light reaches us 

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The Solar Neighborhood 

The region of space around us, beyond the edge of the solar system: 

‐“sea” of stars visible in the night sky  

Typical Distances between stars: ‐several light years  (1ly. = 9.47x1012 km)  

         https://apod.nasa.gov/apod/ap000611.html 

 

Scale model:  Sun = size of ping‐pong ball 

  

 

 

 http://www.atlasoftheuniverse.com/ 

 http://www.atlasoftheuniverse.com/ 

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The (Milky Way) Galaxy 

A huge rotating system including: ‐100,000,000,000 stars (& their planets) ‐gas & dust clouds, black holes etc. ‐roughly 100,000 light years across  

 http://www.smithsonianmag.com/photocontest/10th‐annual/10th‐Annual‐Photo‐Contest‐Finalists‐Natural‐World‐194333591.html 

 

 Panorama over Yosemite National Park    http://apod.nasa.gov/apod/ap140502.html  

 

 http://www.slate.com/blogs/bad_astronomy/2012/12/02/the_milky_way_and_the_lighthouse_photos_from_australia.html 

 

 

 

All the objects in the MW move around the center 

  ‐ Sun and solar system take roughly 225 million years to orbit around the galaxy once! 

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The Local Group 

A large region of space containing: ‐The Milky Way Galaxy ‐The Andromeda Galaxy ‐over 30 smaller galaxies ‐roughly 5 million light years across 

 

 http://www.atlasoftheuniverse.com/ 

 

 M31, Andromeda Galaxy http://apod.nasa.gov/apod/ap090510.html 

 

M33, Triangulum Galaxy    Small/Large Magellanic Clouds

The Local (Virgo) Supercluster 

An enormous region of space containing: ‐The Local Group ‐The Virgo Cluster ‐up to 100 other galaxy clusters ‐up to 50 ‐ 100 million light years in size 

 http://www.atlasoftheuniverse.com/ 

 

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The Universe An immense (and possibly infinite) “sea” of galaxy clusters and superclusters   ‐ visible size roughly 13.5 ‐ 14 billion light 

 years 

 http://www.atlasoftheuniverse.com/ 

Hubble Deep Field Survey 

 

Hubble Deep Field with Redshifts 

 z = 1.0  r = 7.8 billion ly        z = 4.0; r = 12.0 billion ly

 http://www.slate.com/blogs/bad_astronomy/2011/12/22/star_factory_at_the_edge_of_the_universe.html  

Most distant object ever observed!! z = 11.9; r = 13.3 billion ly  

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 http://www.atlasoftheuniverse.com/