Astronomy 101 The Solar System Tuesday Thursday 2

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Astronomy 101 The Solar System Tuesday, Thursday 2: 30 -3: 45 pm Hasbrouck 20

Astronomy 101 The Solar System Tuesday, Thursday 2: 30 -3: 45 pm Hasbrouck 20 Tom Burbine tomburbine@astro. umass. edu

Course • Course Website: – http: //blogs. umass. edu/astron 101 -tburbine/ • Textbook: –

Course • Course Website: – http: //blogs. umass. edu/astron 101 -tburbine/ • Textbook: – Pathways to Astronomy (2 nd Edition) by Stephen Schneider and Thomas Arny. • You also will need a calculator.

Office Hours • Mine • Tuesday, Thursday - 1: 15 -2: 15 pm •

Office Hours • Mine • Tuesday, Thursday - 1: 15 -2: 15 pm • Lederle Graduate Research Tower C 632 • Neil • Tuesday, Thursday - 11 am-noon • Lederle Graduate Research Tower B 619 -O

Homework • We will use Spark • https: //spark. oit. umass. edu/webct/logon. Display. d

Homework • We will use Spark • https: //spark. oit. umass. edu/webct/logon. Display. d owebct • Homework will be due approximately twice a week • I will drop the lowest homework score.

HW #2, #3, #4 • I will go over the answers • http: //blogs.

HW #2, #3, #4 • I will go over the answers • http: //blogs. umass. edu/astron 101 -tburbine

Exam #1 • • • Review questions are online Thursday 40 questions Multiple choice

Exam #1 • • • Review questions are online Thursday 40 questions Multiple choice and True/False Review session: – Wednesday 6 -7 pm in Hasbrouck 20

http: //www. hulu. com/watch/63319/cosmos-the-harmony-of-the-worlds

http: //www. hulu. com/watch/63319/cosmos-the-harmony-of-the-worlds

Acceleration • Acceleration is when your velocity is changing • Velocity not changing, no

Acceleration • Acceleration is when your velocity is changing • Velocity not changing, no acceleration

Acceleration • • • a = ∆v/∆t Car is travelling at 10 m/s Increases

Acceleration • • • a = ∆v/∆t Car is travelling at 10 m/s Increases its speed to 30 m/s over 5 seconds a = (30 m/s – 10 m/s)/5 seconds a = 4 m/s 2

Difference between mass and weight • Mass is the amount of matter in your

Difference between mass and weight • Mass is the amount of matter in your body • Weight is the amount of force acting on your body • So on the Moon, you would have the same mass as on Earth but weigh less on the Moon since the Moon is less massive than Earth

Isaac Newton (1642 -1727) • Supposedly saw an apple fall to the ground •

Isaac Newton (1642 -1727) • Supposedly saw an apple fall to the ground • He then understood that gravity was universal, meaning it affected both the planets and us on Earth • Came up with 3 Laws of Motion

Force • Force – anything that can cause a body to change velocity

Force • Force – anything that can cause a body to change velocity

Newton’s st 1 Law • In the absence of a net (overall) force acting

Newton’s st 1 Law • In the absence of a net (overall) force acting upon it, an object moves with a constant velocity • An object at rest remains at rest • An object in motion tends to remain in motion unless a force is acting upon it

Why do things on Earth not remain in motion?

Why do things on Earth not remain in motion?

Why do things on Earth not remain in motion? • Friction

Why do things on Earth not remain in motion? • Friction

Newton’s • • • nd 2 Law Force = mass x acceleration Units of

Newton’s • • • nd 2 Law Force = mass x acceleration Units of Force kg m/s 2 = newton So much do you weigh Say your mass is 100 kg F = 100 kg x 9. 8 m/s 2 F = 980 Newtons

Newton’s rd 3 Law • For any force, there is an equal and opposite

Newton’s rd 3 Law • For any force, there is an equal and opposite reaction force • Gravity is holding you on the ground • The ground is also pushing back up on you with the same amount of force

http: //www. vshiksha. com/system/files/u 1/pslvc 6 -rocket. jpg

http: //www. vshiksha. com/system/files/u 1/pslvc 6 -rocket. jpg

Newton’s Universal Law of Gravitation • Every mass attracts every other mass through the

Newton’s Universal Law of Gravitation • Every mass attracts every other mass through the force called gravity • Newton came up with this formula F = G M 1 M 2 r 2 M 1, M 2 are the masses of the two objects r is the distance between the objects G = constant = 6. 67 x 10 -11 m 3/(kg s 2)

So what should you know about this formula F = G M 1 M

So what should you know about this formula F = G M 1 M 2 r 2 • The force of attraction between any two objects is directly proportional to the product of their masses • The force of attraction between two objects decreases with the square of the distance between their centers • G is a very small number

What is the attraction of two people in this room? F = G M

What is the attraction of two people in this room? F = G M 1 M 2 r 2 • • • Say their masses are both 100 kg Their distances are 10 meters apart F = 6. 67 x 10 -11 m 3/(kg s 2) * 100*100 kg 2/(10*10 m 2) F = 6. 67 x 10 -9 N = 0. 000067 N Remember the person weighs 980 N

Any Questions?

Any Questions?