Astronomy: Newton's and Kepler's Laws

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Questions and Answers

What does Newton's First Law state?

An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.

What does Newton's Second Law state?

The change of motion of a body is proportional to and in the direction of the force acting on it.

What is Newton's Law of Gravitation?

$f1 = f2 = g * (m1*m2) / r^2$

Objects fall at which rate, independent of mass?

<p>The same rate</p> Signup and view all the answers

What does Kepler's Third Law state?

<p>The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.</p> Signup and view all the answers

What is Angular Momentum?

<p>Rotational momentum of a spinning or orbiting object</p> Signup and view all the answers

What is light?

<p>A particle and a wave</p> Signup and view all the answers

What is another term for light?

<p>Electromagnetic radiation</p> Signup and view all the answers

List differences between light and sound waves.

<ol> <li>Light is a transverse wave sound is a longitudinal wave. 2. Light can be polarised. 3. The speed of Light is much faster than sound. light 300,000,000 m per s. Sound 340 m per s. 4. Sound requires a medium to travel through.</li> </ol> Signup and view all the answers

Define wavelength.

<p>Horizontal distance between the crests or between the troughs of two adjacent waves (measured in meters)</p> Signup and view all the answers

Define Frequency.

<p>The number of complete wavelengths that pass a point in a given time (Measured in Hertz)</p> Signup and view all the answers

What is a photon?

<p>A particle of light</p> Signup and view all the answers

List two distinct ways to observe stellar spectra.

<ol> <li>Spectral Curves (or blackbody curves) 2. Spectral Lines (absorption or emission)</li> </ol> Signup and view all the answers

What is Blackbody Radiation?

<p>Emission of light from hot objects</p> Signup and view all the answers

What is an Atomic Nucleus?

<p>An atom's central core, containing protons and neutrons.</p> Signup and view all the answers

What are Atomic Orbitals?

<p>The regions around the nucleus within which the electrons have the highest probability of being found</p> Signup and view all the answers

What defines an element?

<p>Number of protons</p> Signup and view all the answers

What defines an isotope?

<p>Number of neutrons</p> Signup and view all the answers

When is an atom "neutral", a "positive ion", and a "negative ion"?

<p>p=e: neutral atom; p&gt;e: positive ion; p</p> Signup and view all the answers

What is Newton's First Law?

<p>An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.</p> Signup and view all the answers

What is Newton's Second Law?

<p>The change of motion of a body is proportional to and in the direction of the force acting on it.</p> Signup and view all the answers

What is Kepler's Third Law?

<p>The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.</p> Signup and view all the answers

What are the differences between light and sound waves?

<ol> <li>Light is a transverse wave sound is a longitudinal wave. 2. Light can be polarised. 3. The speed of Light is much faster than sound. light 300,000,000 m per s. Sound 340 m per s. 4. Sound requires a medium to travel through.</li> </ol> Signup and view all the answers

What is wavelength?

<p>Horizontal distance between the crests or between the troughs of two adjacent waves (measured in meters)</p> Signup and view all the answers

What is frequency?

<p>The number of complete wavelengths that pass a point in a given time (Measured in Hertz)</p> Signup and view all the answers

What are 2 distinct ways to observe stellar spectra?

<p>1.Spectral Curves (or blackbody curves) 2.Spectral Lines (absorption or emission)</p> Signup and view all the answers

What are the conditions for a neutral atom, a positive ion, and a negative ion, in terms of protons (p) and electrons (e)?

<p>p=e: neutral atom, p&gt;e: positive ion, p&lt;e: negative ion</p> Signup and view all the answers

Define angular momentum.

<p>Rotational momentum of a spinning or orbiting object</p> Signup and view all the answers

Define photon.

<p>A particle of light</p> Signup and view all the answers

Define blackbody radiation.

<p>Emission of light from hot objects</p> Signup and view all the answers

Define atomic nucleus.

<p>An atom's central core, containing protons and neutrons.</p> Signup and view all the answers

Define atomic orbitals.

<p>The regions around the nucleus within which the electrons have the highest probability of being found</p> Signup and view all the answers

Define element.

<p>Number of protons</p> Signup and view all the answers

Describe the relationship between protons (p), electrons (e) and a neutral atom, positive ion and negative ion

<p>p=e: neutral atom, p&gt;e: positive ion, p&lt;e: negative ion</p> Signup and view all the answers

Flashcards

Newton's First Law

An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.

Newton's Second Law

The change of motion of a body is proportional to and in the direction of the force acting on it.

Newton's Third Law

For every action there is an equal and opposite reaction

Newton's Law of Gravitation

f1 = f2 = g * (m1*m2) / r^2

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The same rate

Objects fall at the same rate, independent of mass

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Kepler's First Law

The orbit of each planet around the Sun is an ellipse with the Sun at one focus.

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Kepler's Second Law

A line joining a planet and the sun sweeps out equal areas in equal intervals of time

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Kepler's Third Law

The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.

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Angular Momentum

Rotational momentum of a spinning or orbiting object

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What is Light?

A particle and a wave

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What is another term for light?

Electromagnetic radiation

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Differences between light and sounds waves

  1. Light is a transverse wave sound is a longitudinal wave. 2. Light can be polarised. 3. The speed of Light is much faster than sound. light 300,000,000 m per s. Sound 340 m per s. 4. Sound requires a medium to travel through.
Signup and view all the flashcards

Wavelength

Horizontal distance between the crests or between the troughs of two adjacent waves (measured in meters)

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Frequency

The number of complete wavelengths that pass a point in a given time (Measured in Hertz)

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Photon

A particle of light

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2 Distinct Ways to Observe Stellar Spectra

1.Spectral Curves (or blackbody curves) 2.Spectral Lines (absorption or emission)

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Blackbody Radiation

Emission of light from hot objects

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Atomic Nucleus

An atom's central core, containing protons and neutrons.

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Atomic Orbitals

The regions around the nucleus within which the electrons have the highest probability of being found

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Element

Number of protons

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Isotope

Number of neutrons

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Study Notes

  • Study notes on Astronomy Exam 2

Newton's First Law

  • An object will remain at rest or in motion at a constant speed and direction unless acted upon by an external, unbalanced force.

Newton's Second Law

  • A body's change in motion is proportional to the force acting on it and occurs in the direction of that force.

Newton's Third Law

  • Every action has an equal and opposite reaction.

Newton's Law of Gravitation

  • The gravitational force (f) between two objects is calculated as: f1 = f2 = g * (m1*m2) / r^2

Rate of Falling Objects

  • Objects fall at the same rate, regardless of their mass.

Kepler's First Law

  • Planets orbit the Sun in an ellipse, with the Sun at one focus.

Kepler's Second Law

  • A line connecting a planet to the Sun sweeps out equal areas during equal time intervals.

Kepler's Third Law

  • The square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit.

Angular Momentum

  • This is the rotational momentum of an object that is either spinning or orbiting.

Nature of Light

  • Light behaves as both a particle and a wave.

Light

  • Light can also be referred to as electromagnetic radiation.

Light Vs Sound Waves

  • Light is a transverse wave, while sound is a longitudinal wave.
  • Light can be polarized, but sound cannot.
  • Light travels much faster than sound with light at 300,000,000 m/s, sound at 340 m/s.
  • Sound requires a medium to propagate, light does not.

Wavelength

  • The distance between crests or troughs of adjacent waves and is measured in meters.

Frequency

  • The number of complete wavelengths passing a point per unit time, measured in Hertz.

Photon

  • A photon is a particle of light.

Observing Stellar Spectra

  • Stellar spectra can be observed through spectral curves (blackbody curves) and spectral lines (absorption or emission).

Blackbody Radiation

  • This refers to the emission of light from hot objects.

Atomic Nucleus

  • The central core of an atom which contains protons and neutrons.

Atomic Orbitals

  • Regions around the nucleus where electrons are most likely to be found.

Element

  • Defined by its number of protons.

Isotope

  • Defined by its number of neutrons.

Atom Electrical Charge

  • p=e: Atom is neutral
  • p>e: Atom is positively charged
  • p

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