astronomy = the study of the universe

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tronomy = the study of the universe Astro = star Centr = center Geo = earth Retro = back Pre = before Peri = around Mar = ocean Terre = ground Sol = sun Chrom = color pro = first

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Astronomy = the study of the universe. Astro = star Centr = center Geo = earth Retro = back Pre = before Peri = around Mar = ocean Terre = ground Sol = sun Chrom = color pro = first. Astronomical History!. Geocentric Model = moon, sun and planets orbit Earth. - PowerPoint PPT Presentation

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Page 1: Astronomy = the study of the universe

Astronomy = the study of the universe

Astro = starCentr = centerGeo = earthRetro = backPre = beforePeri = aroundMar = oceanTerre = groundSol = sunChrom = colorpro = first

Page 2: Astronomy = the study of the universe

Astronomical History!

• Geocentric Model = moon, sun and planets orbit Earth.

Page 3: Astronomy = the study of the universe

Astronomical History!

• Heliocentric Model = Earth and other planets orbit sun.

Page 4: Astronomy = the study of the universe

Astronomical History!

• Ptolemaic System = Planets orbit Earth, but seemed to exhibit retrograde motion.

Page 5: Astronomy = the study of the universe

Astronomical History!Copernicus:

Earth is a planet that

orbits the sun.

Brahe: Yes, but my observations are much more

precise.

Kepler: No, my 3 laws of planetary

motion prove that Brahe is

wrong.

Galileo: Well, here is how the planets and their satellites

move.

Newton: The planets are held

into a circle by the gravity of the sun.

Page 6: Astronomy = the study of the universe

Earth – Moon - Sun

Rotation = spinningRevolution = going around another object

Earth Rotating http://svs.gsfc.nasa.gov/vis/a000000/a001300/a001374/index.html

Perihelion Aphelion

CLOSEST FARTHEST

Page 7: Astronomy = the study of the universe

SEASONS

Plane of the Ecliptic = reference plane that runs from pole to pole.

Plane is tilted about 23.5o.

Seasons are result of the tilt.

Page 8: Astronomy = the study of the universe

More Earth Movement

Precession = very slow wobbling

http://earthobservatory.nasa.gov/Features/Milankovitch/Images/milankovitch_precess_high.mov

Page 9: Astronomy = the study of the universe

Earth - Moon

Perigee = moon is closest to earthApogee = moon is farthest from earth

Page 10: Astronomy = the study of the universe

Phases of the Moon

http://videos.howstuffworks.com/hsw/10001-the-moon-phases-video.htm

Page 11: Astronomy = the study of the universe

NAME THAT PHASE!

Page 12: Astronomy = the study of the universe

ECLIPSE

Solar eclipse = moon is between earth and sun (like the background here!) and casts a shadow on Earth.Lunar eclipse = Earth moves between sun and moon and casts shadow on moon.

Page 13: Astronomy = the study of the universe

Man on the Moon

http://news.sky.com/skynews/Home/World-News/Nasa-Releases-Footage-Of-Moon-Landing-When-Astronaut-Neil-Armstong-Took-First-Steps-On-July-20-1969/Article/200907315338603

Page 14: Astronomy = the study of the universe

Earth’s Moon

• The Only Natural Satellite• 1/4th diameter of Earth• Apollo moon mission 1969-1972

• Gravity 1/6th that of Earth• 150 lb person = 25 lbs

Page 15: Astronomy = the study of the universe

Craters • round depressions• produced by impacts

Impact by meteor. Compresses surface material.

Rebound splash of ejecta. Uplift of deep rock in center.

Page 16: Astronomy = the study of the universe
Page 17: Astronomy = the study of the universe

Major Topographic features of the Moon:

Highlands = light colored areas (almost as high as Mt. Everest!)Mare (Maria, pl.) = dark smooth areas (ancient beds of lava)

Rilles are valleys or trenches.Regolith = soil-like layer

Page 18: Astronomy = the study of the universe

Lunar History

When solar system was forming, a body the size of Mars impacted Earth and the debris shot into space. One piece was our Moon.

How the Moon Formed http://videos.howstuffworks.com/hsw/9998-the-moon-formation-video.htm

Page 19: Astronomy = the study of the universe

The Solar System

Terrestrial Planet = small and rocky (inner planets)Jovian Planet = large gaseous (outer planets)

http://player.discoveryeducation.com/index.cfm?guidAssetId=21B610C4-B1BB-40E0-8760-825A41B19E12&blnFromSearch=1&productcode=US

Nebular Theory = sun and planets formed from a rotating disk of dust and gases.

Planetesimals = small, irregular-shaped bodies that collided and clumped together to form the planets.

Formation of the Solar System

Page 20: Astronomy = the study of the universe

Asteroids = small, rocky bodies floating in space(Largest, Ceres, is about 1000 km in diameter!)

Comets = pieces of rocky and metallic materials held togetherby frozen gases like water, ammonia, methane, etc.

(Some take hundreds of thousands of years to make one orbit.)

Small Pieces (w/Quiz) http://player.discoveryeducation.com/index.cfm?guidAssetId=BD722E4D-32D2-4342-B475-F031BFDC4EEC&blnFromSearch=1&productcode=US

Page 21: Astronomy = the study of the universe

Coma = the glowing head of a comet produced when the sun begins vaporizing the comet’s frozen gases.Tail = stream of glowing vaporizing gases

Halley’s Comet76-yr-orbit

Page 22: Astronomy = the study of the universe

Kuiper Belt = disc-shaped region beyond Neptune where short-orbital comets originate.

Oort Cloud = area spreading in all directions from the sun where long-orbital comets originate.

Page 23: Astronomy = the study of the universe

METEORS!Meteoroid

• small, solid particle• travels through space• origination• interplanetary debris• asteroid belt material• remains of comets

Meteor

• meteoroid that enters Earth’s atmosphere• Meteor Shower = a group of meteors traveling in the same direction

Meteor in Peru 2007 http://news.bbc.co.uk/player/nol/newsid_7000000/newsid_7002300/7002376.stm?bw=bb&mp=wm&asb=1&news=1&ms3=54&ms_javascript=true&bbcws=2

Page 24: Astronomy = the study of the universe

The SUNPhotosphere = visible surface (90% hydrogen)

Chromosphere = thin layer of hot gases (can see during solar eclipse)

Corona = weak outermost layer (extends 1 million km)

Solar wind = streams of protons and electrons

Page 25: Astronomy = the study of the universe

Convective Zone

Radiative Zone

Core

Photosphere

Chromosphere

Corona

Earth

Page 26: Astronomy = the study of the universe

Activity of the Sun:

Sunspots = appear dark because they are cooler than the rest of the sun. http://www.windows.ucar.edu/tour/link=/sun/atmosphere/

sun_rotate_anim_jan2005.html&edu=high

Prominences = large cloudlike structures consisting of chromospheric gases.

Page 27: Astronomy = the study of the universe

Solar Flares

• explosive events• last about an hour• sudden brightening above a sunspot cluster• release enormous amounts of energy• ejects atomic particles• produce auroras (northern lights)

http://images.google.com/imgres?imgurl=http://earthobservatory.nasa.gov/images/imagerecords/3000/3912/flare_soh_2003301.jpg&imgrefurl=http://earthobservatory.nasa.gov/IOTD/view.php%3Fid%3D3912&usg=__1KWUaN-ZdTALrPPKRSxiynbT1xU=&h=865&w=540&sz=74&hl=en&start=3&um=1&itbs=1&tbnid=jLzIYZNVqdx_VM:&tbnh=145&tbnw=91&prev=/images%3Fq%3Dsolar%2Bflare%2Banimation%26ndsp%3D20%26hl%3Den%26safe%3Dactive%26rls%3Dcom.microsoft:en-us%26um%3D1

http://images.google.com/imgres?imgurl=http://veimages.gsfc.nasa.gov/10194/a001168_pre.jpg&imgrefurl=http://visibleearth.nasa.gov/view_rec.php%3Fid%3D10194&usg=__0rK1487FipNjvZgrwD7bE1yTeO8=&h=242&w=320&sz=7&hl=en&start=13&um=1&itbs=1&tbnid=rfP8CkCb5ln2KM:&tbnh=89&tbnw=118&prev=/images%3Fq%3Dsolar%2Bflare%2Banimation%26ndsp%3D20%26hl%3Den%26safe%3Dactive%26rls%3Dcom.microsoft:en-us%26um%3D1

Page 28: Astronomy = the study of the universe

It’s how far??!!

1 Light Year = how far light travels in one year. Light travels at 299,792,458 m/s so in one year light goes 5.88 trillion (5.88 × 1012) miles.

1 A.U. (Astronomical Unit) is the distance from the Earth to the Sun which is 150 million km (93 million miles).

Page 29: Astronomy = the study of the universe

Earth’s diameter = 7,926 miles

Page 30: Astronomy = the study of the universe
Page 31: Astronomy = the study of the universe

  

   ANTARES IS THE 15TH BRIGHTEST STAR IN THE SKY. IT IS MORE THAN 1000 LIGHT YEARS AWAY. THIS IS A HUBBLE TELESCOPE ULTRA DEEP FIELD INFRARED VIEW OF COUNTLESS 'ENTIRE' GALAXIES BILLIONS OF LIGHT-YEARS AWAY. BELOW IS A CLOSE UP OF ONE OF THE DARKEST REGIONS OF THE PHOTO ABOVE.

   

Sun’s diameter = 870,000 miles

Page 32: Astronomy = the study of the universe

Sirius is the brightest star in the night-time sky. It is located in the constellation Canis Major. It is 8.5 light years away. Pollux is 33.7 light years away. Arcturus is 36.7 light years away.

Page 33: Astronomy = the study of the universe

ANTARES IS THE 15TH BRIGHTEST STAR IN THE SKY. IT IS MORE THAN 1000 LIGHT YEARS AWAY.

Page 34: Astronomy = the study of the universe

How to Build a Star

1. Locate a nebula (cloud of dust and gases).

Page 35: Astronomy = the study of the universe

How to Build a Star

2. Contract your nebula.

Page 36: Astronomy = the study of the universe

How to Build a Star

3. Squeeze your nebula more using gravity.

Page 37: Astronomy = the study of the universe

How to Build a Star

4. Convert the gravitational energy into heat energy.

Page 38: Astronomy = the study of the universe

How to Build a Star

5. Conversion gives you a protostar.

Page 39: Astronomy = the study of the universe

How to Build a Star

6. Continue to squeeze until the core reaches 10 million K of pressure.

Congratulations…It’s a Star!

Page 40: Astronomy = the study of the universe

How to Raise a Star

1. Provide support and guidance while your young star struggles with internal gas pressures and forces of gravity.

Page 41: Astronomy = the study of the universe

How to Raise a Star

2. Have your star identified by a star doctor to determine its color.

Blue stars burn fast and die quickly in about 3 million years.Yellow stars brun slowly and live about 10 billion years.

Page 42: Astronomy = the study of the universe

How to Raise a Star

3. Provide senior care as your star reaches the red-giant stage and its core is consumed.

Page 43: Astronomy = the study of the universe

How to Raise a Star

4. Apply gravity to offset the loss of fuel.

Page 44: Astronomy = the study of the universe

The Death of a Star

1. Prepare for the eventual collapse of your star by gravity.

Page 45: Astronomy = the study of the universe

The Death of a Star

2. If your star was a low mass star, care for it as it collapses into a white dwarf.

Page 46: Astronomy = the study of the universe

The Death of a Star

3. If your star was a medium mass star, care for it as it bloats into a planetary nebula.

Page 47: Astronomy = the study of the universe

The Death of a Star

4. If your star was a massive star, run away! A supernova is coming!

Page 48: Astronomy = the study of the universe

The Death of a Star

5. When your star goes supernova, prepare for a black hole.

Black holes are made when pieces of stars 3x bigger than our sun collapse making smaller objects with immense gravitational pulls. The gravity is so strong that not even light can escape.

Page 49: Astronomy = the study of the universe

Home Sweet Home

Galaxy = group of dust, stars, and gases held together by gravity.

Circinus GalaxyAndromeda Galaxy

Sombrero Galaxy

Methusala Galaxy

Cartwheel Galaxy

Page 50: Astronomy = the study of the universe

Home Sweet Home

Milky Way Galaxy

ASSIGNMENT:PH CH 22, 23, 24, 25

Google Earth to space