Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126...

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Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: [email protected] Webpage: http://itscience.tsu.edu/ma Department of Computer Science & Physics Texas Southern University, Houston Nov. 8, 2004

Transcript of Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126...

Page 1: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

Phys141 Principles of Physical Science

Chapter 15 The Solar System

Instructor: Li Ma

Office: NBC 126Phone: (713) 313-7028Email: [email protected]

Webpage: http://itscience.tsu.edu/ma

Department of Computer Science & PhysicsTexas Southern University, Houston

Nov. 8, 2004

Page 2: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

Topics To Be Discussed

An Overview The Planet Earth The Terrestrial Planets The Jovian Planets and Pluto Skip §15.5 – §15.7

Page 3: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Solar System

The universe is the totality of all matter, energy, space and time

Astronomy is the study of the universe Solar system is a complex system of moving

masses All these moving masses are held together by

gravitational forces Sun: a star at the center of solar system, the

dominant mass

Page 4: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Solar System (cont)

Objects revolving around the Sun:– 9 rotating planets– over 70 satellites (moons)– thousands of asteroids– comets, meteoroids, interplanetary dust particles,

gases, and solar wind composed of charged particles

Page 5: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Model of Solar System

Geocentric model: Earth-centered model Heliocentric model: Sun-centered model Kepler’s first law: law of elliptical paths

– All planets move in elliptical paths around the Sun at one focus of the ellipse

Kepler’s second law: law of equal areas– An imaginary line (radial vector) joining a planet to

the Sun sweeps out equal area in equal periods of time

Page 6: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Model of Solar System (cont)

Kepler’s third law: harmonic law– The square of the sidereal period of a planet is

proportional to the cube of its semimajor axis (one half the major axis)

(period)2 ∞ (semimajor axis)3

T2 = kR3

– Sidereal period (T): time of one revolution with respect to a star, the orbital period with respect to the stars – the true period of revolution

Page 7: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Model of Solar System (cont)

For the Earth, time of one revolution with respect to the Sun is one year (T = 1 y)

Astronomical Unit (AU): average distance between the Earth and the Sun– 1 AU = 1.5 x 108 km

So, k = 1 y2/AU3, and same for all planets Table 15.1 on page 384 e.g. R = 1.52 AU, T = ?

Page 8: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

Planets in Solar System

Terrestrial planets: inner planets– Mercury, Venus, Earth, and Mars

Jovian planets: outer planets– Jupiter, Saturn, Uranus, and Neptune

Pluto: does not resemble the Earth or Jupiter, has the smallest diameter

Prograde motion: west-to-east revolution Retrograde motion: east-to-west revolution

Page 9: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Planet Earth

The Earth is a solid, spherical, rocky body with oceans and an atmosphere.

In our solar system, the Earth is the only planet with large amounts of surface water, an atmosphere that contains oxygen, a temperate climate, and living organisms

The Earth is an oblate spheroid, fattened at the poles and bulging at the equator

Page 10: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Planet Earth (cont)

The Earth is undergoing several motions simultaneously– The daily rotation on its axis– The annual revolution around the Sun– Procession

Rotation: spinning on an inter axis Revolution: the movement of one mass

around another

Page 11: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Planet Earth (cont)

The Earth rotates eastward around a central internal axis that is tilted 23.5° from the line perpendicular to its orbital plane

– The Foucault pendulum is an experimental proof of the Earth’s rotation on its axis

The Earth revolves eastward around the Sun

– The observation of parallax

– The telescope observation of systematic change in position of stars annually

Page 12: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Planet Earth (cont)

The 23.5° tilt of the axis and the revolution of the Earth around the Sun are the reason for the four seasons we experience annually

Page 13: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Terrestrial Planets

Mercury, Venus, Earth, and Mars Relatively small in size and mass Composed of rocky material and metals Relatively dense and have solid surface and

weak magnetic fields Relatively close to the Sun None has a ring system

Page 14: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Terrestrial Planets (cont)

Only the Earth and Mars have moons Only the Earth has surface water and an

atmosphere that is 21% oxygen, others have no free oxygen in their atmosphere

Mercury: the closest planet to the Sun, has the shortest period of revolution, is the fast-moving planet

Page 15: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Terrestrial Planets (cont)

Venus: our closest planetary neighbor, third brightest object in the sky, exceeded only by the Sun and our Moon

Mars: has a reddish color when viewed from the Earth, is the planet that most closely resembles the Earth; unmanned spacecrafts have been sent to Mars, a manned landing may be sent in future

Page 16: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Jovian Planets & Pluto

Jupiter, Saturn, Uranus, and Neptune large in size compared with the terrestrial

planets gaseous, no solid surface, composed mainly

of hydrogen and helium All have a very low density and have strong

magnetic fields have many rings and moons Very distant from the Sun with orbits far apart

Page 17: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Jovian Planets & Pluto (cont)

Jupiter: the largest planet of the solar system, in both volume and mass, has many moons

Saturn: has three prominent rings, three spacecrafts have visited it, another is on its way

Uranus: has a ring system that is very thin, has over 20 moons

Page 18: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

The Jovian Planets & Pluto (cont)

Neptune: regarded as a twin to Uranus due to their similarity in size, composition of their atmospheres and internal structure

Pluto: the most distant planet from the Sun, the only planet that has not been visited by a space probe

Page 19: Phys141 Principles of Physical Science Chapter 15 The Solar System Instructor: Li Ma Office: NBC 126 Phone: (713) 313-7028 Email: malx@tsu.edumalx@tsu.edu.

Assignment

Homework Assignment– Review Questions (page 412 – 413):

1,3,9,11,13,25,42

– Exercises (page 414): 2,4

– It’s due Monday, 11/22/04

Reading Assignment– Chapter 16