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Transcript of 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400...

Page 1: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.
Page 2: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

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The Sun & Other Stars

Page 3: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

Row 1, Col 1

This Law tells us the distance of a planet from the Sun if we know

its period.

What is Keplers Third Law?

Page 4: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

2,1

The method has found most of the known extrasolar planets.

What is the radial velocity method?

Page 5: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

3,1

Gaseous planets and icy bodies formed beyond this location

in our solar system.

What is the Frost Line?

Page 6: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

4,1

This process built the planet we are standing on during the

formation of the solar system

What is accretion?

Page 7: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

5,1

This causes the seasons on Pluto

What is the eccentricity of Pluto (or) What is the distance of Pluto from the Sun?

Page 8: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

1,3

This event leaves a neutron star behind.

What is a massive star supernova?

Page 9: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

2,3

This allows us to determine the age of a cluster of stars.

What is the main sequence turn off (TO) point?

Page 10: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

3,3

This is the second longest living type of star on the

main sequence.

What is a K Type Main Sequence Star?

Page 11: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

4,3

This supports a White Dwarf against gravitational collapse.

What is electron degeneracy pressure?

Page 12: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

5,3

This is the first thing that happens when a star leaves the

main sequence.

What is a contracting core?

Page 13: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

1,2

This type of radiation has the lowest energy.

What are radio waves?

Page 14: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

2,2

This tells us how the peak Wavelength of a blackbodyChanges with temperature

What is Wien’s Law?

Page 15: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

3,2

This tells us the distance to the nearest star cluster.

What is stellar parallax?

Page 16: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

4,2

This tells us the composition of acool low density gas.

What is an absorption spectrum?

Page 17: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

5,2

This relation tells us how to determine mass from a rotation

curve

What is the orbital velocity Law

(or orbital velocity-radius-mass relation)?

Page 18: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

1,4

The thirty or so galaxies around us belong to one of these.

What is a galaxy group.

Page 19: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

2,4

These are the size of a solar system and more luminous than

a galaxy

What are Active Galactic Nuclei (AGN or Quasars)?

Page 20: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

3,4

Spiral galaxies of this type are more commonly found at small

lookback times.

What is a spiral galaxy with a bar?

Page 21: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

4,4

These galaxies have very high rates of star formation.

What are starburst (or merging) galaxies?

Page 22: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

5,4

This is something that increases as a galaxy ages.

What is metallicity (C,O,Fe) ?

Page 23: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

1,5

It tells us the distance to an object based on its Doppler shift.

What is the Hubble Law?

Page 24: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

2,5

This is all around us and is evidence that the Universe started with a big bang.

What is the Cosmic Microwave Background (CMB) ?

Page 25: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

3,5

This relation is used to find the distances to nearby galaxies.

What is the Cephied Period-Luminosity relation?

Page 26: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

4,5

These objects are used to find the distances to very remote

galaxies.

What are white dwarf supernovae?

Page 27: 100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.

1,5

This number tells us how the Universe will come to an end.

What is the critical density of the Universe?


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Jeopardy $500 $400 $300 $200 $100 $500 $400 $300 $200 $100 $500 $400 $300 $200 $400 $300 $200 $100 $500 $400 $300 $200 $100 $500 $400 $300 $200 $100 Business.

Jeopardy $500 $400 $300 $200 $100 $500 $400 $300 $200 $100 $500 $400 $300 $200 $400 $300 $200 $100 $500 $400 $300 $200 $100 $500 $400 $300 $200 $100 Business.

100 200 400 300 400 ExcavationsFallsScaffoldsCranes 300 200 400 200 100 500 100.

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100 200 400 300 400 GeographyCivicsEconomicsHistory 300 200 400 200 100 500 100.

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Transformations SymmetryAsymptotesFunctionsSketching 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400.

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MatterWaterpHBonding Miscellaneous 100 200 300 400 100 200 300 400 200 300 400 200 300 400 100.

SOUTHEAST TASMANIA GROUNDWATER MAP · 700 600 500 100 100 200 200 200 400 500 700 100 100 100 100 100 200 200 200 200 400 400 200 300 200 300 400 200 300 400 500 600 100 100 100 100

SOUTHEAST TASMANIA GROUNDWATER MAP · 700 600 500 100 100 200 200 200 400 500 700 100 100 100 100 100 200 200 200 200 400 400 200 300 200 300 400 200 300 400 500 600 100 100 100 100

Proteins $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100.

Proteins $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100.

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100 200 400 300 400 1234 300 200 400 200 100 500 100.

100 200 400 300 400 CATEGORY 300 200 400 200 100 500 100.

100 200 400 300 400 CATEGORY 300 200 400 200 100 500 100.

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