Thing 1
• Very Weak
• Predictable Force
• Helped form the universe
• Property of mass/matter
• Proportional to mass
• Affected by (Net) Force
Thing 2
Thing 1
• Very Weak
• Predictable Force
• Helped form the universe
• Constant presence
• Acts on all matter in the
universe
• Distortion of space/time
• Property of mass/matter
• Proportional to mass
• Affected by (Net) Force
• Resistance to change in velocity
• An object will not speed up on its
own
• An object will not slow down on
its own
Thing 2
Thing 1
• Very Weak
• Predictable Force
• Helped form the universe
• Constant presence
• Acts on all matter in the
universe
• Distortion of space/time
• Function of mass and distance
• A push
• A pull
• Property of mass/matter
• Proportional to mass
• Affected by (Net) Force
• Resistance to change in velocity
• An object will not speed up on its
own
• An object will not slow down on
its own
• An object will not start moving
on its own
• An object will not stop moving on
its own
• Idea first proposed by Galileo
Thing 2
Thing 1
• Very Weak
• Predictable Force
• Helped form the universe
• Constant presence
• Acts on all matter in the
universe
• Distortion of space/time
• Function of mass and distance
• A push
• A pull
• Keeps you on the Earth
• Keeps the Earth around the
sun
• Idea first proposed by Newton
• Einstein
• Property of mass/matter
• Proportional to mass
• Affected by (Net) Force
• Resistance to change in velocity
• An object will not speed up on its
own
• An object will not slow down on its
own
• An object will not start moving on
its own
• An object will not stop moving on
its own
• Idea first proposed by Galileo
• Explained by Newton
• An object in motion will stay in
motion unless acted on by an
outside force
• An object at rest will stay at rest
unless acted on by an outside force
• First Law of Motion
Thing 2
Gravity
• Very Weak
• Predictable Force
• Helped form the universe
• Constant presence
• Acts on all matter in the
universe
• Distortion of space/time
• Function of mass and distance
• A push
• A pull
• Keeps you on the Earth
• Keeps the Earth around the
sun
• Idea first proposed by Newton
• Einstein
• Property of mass/matter
• Proportional to mass
• Affected by (Net) Force
• Resistance to change in velocity
• An object will not speed up on its
own
• An object will not slow down on its
own
• An object will not start moving on
its own
• An object will not stop moving on
its own
• Idea first proposed by Galileo
• Explained by Newton
• An object in motion will stay in
motion unless acted on by an
outside force
• An object at rest will stay at rest
unless acted on by an outside force
• First Law of Motion
Inertia
Microgravity Article
1. First reading: annotate
2. Second reading: complete story strip

Dance of the planets

  • 1.
    Thing 1 • VeryWeak • Predictable Force • Helped form the universe • Property of mass/matter • Proportional to mass • Affected by (Net) Force Thing 2
  • 2.
    Thing 1 • VeryWeak • Predictable Force • Helped form the universe • Constant presence • Acts on all matter in the universe • Distortion of space/time • Property of mass/matter • Proportional to mass • Affected by (Net) Force • Resistance to change in velocity • An object will not speed up on its own • An object will not slow down on its own Thing 2
  • 3.
    Thing 1 • VeryWeak • Predictable Force • Helped form the universe • Constant presence • Acts on all matter in the universe • Distortion of space/time • Function of mass and distance • A push • A pull • Property of mass/matter • Proportional to mass • Affected by (Net) Force • Resistance to change in velocity • An object will not speed up on its own • An object will not slow down on its own • An object will not start moving on its own • An object will not stop moving on its own • Idea first proposed by Galileo Thing 2
  • 4.
    Thing 1 • VeryWeak • Predictable Force • Helped form the universe • Constant presence • Acts on all matter in the universe • Distortion of space/time • Function of mass and distance • A push • A pull • Keeps you on the Earth • Keeps the Earth around the sun • Idea first proposed by Newton • Einstein • Property of mass/matter • Proportional to mass • Affected by (Net) Force • Resistance to change in velocity • An object will not speed up on its own • An object will not slow down on its own • An object will not start moving on its own • An object will not stop moving on its own • Idea first proposed by Galileo • Explained by Newton • An object in motion will stay in motion unless acted on by an outside force • An object at rest will stay at rest unless acted on by an outside force • First Law of Motion Thing 2
  • 5.
    Gravity • Very Weak •Predictable Force • Helped form the universe • Constant presence • Acts on all matter in the universe • Distortion of space/time • Function of mass and distance • A push • A pull • Keeps you on the Earth • Keeps the Earth around the sun • Idea first proposed by Newton • Einstein • Property of mass/matter • Proportional to mass • Affected by (Net) Force • Resistance to change in velocity • An object will not speed up on its own • An object will not slow down on its own • An object will not start moving on its own • An object will not stop moving on its own • Idea first proposed by Galileo • Explained by Newton • An object in motion will stay in motion unless acted on by an outside force • An object at rest will stay at rest unless acted on by an outside force • First Law of Motion Inertia
  • 6.
    Microgravity Article 1. Firstreading: annotate 2. Second reading: complete story strip