பீட்டாஇந்த தளம் தீவிர வளர்ச்சியில் உள்ளது; பிழைகள், விடுபட்ட அம்சங்கள் மற்றும் தரவு இழப்பு அபாயம் உள்ளன. உங்கள் ஆதரவுக்கு நன்றி!

The Solar System

விளையாடிக் கற்றுக்கொள்ளுங்கள்

ஆற்றல் சம்பாதிக்க இந்த கேள்விகளுக்குப் பதிலளியுங்கள், பின்னர் மீன் பிடித்து ஆராயுங்கள். கணக்கு தேவையில்லை.

ஆசிரியர்களுக்கு: The Solar System (Co-ordinated Sciences (Double Award) [CIE], Physics)-க்கான தயாரான பாட ஸ்லைடுகள், திருப்புதல் குறிப்புகள் — உங்கள் பாடத்தில் அவற்றைப் பயன்படுத்தவும், அல்லது மாணவர்கள் நேரலை விளையாட்டாக விளையாடும் ஊடாடும் வகுப்பு செயல்பாடாக தலைப்பை இயக்கவும்.

பாட குறிப்புகள்

The Solar System

  • The Solar System consists of the Sun, eight planets, natural and artificial satellites, and minor planets (including dwarf planets).
  • The Sun is a star at the centre; it contains >99% of the Solar System's mass.
  • The eight planets in order from the Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune.
  • Planets are divided into inner rocky planets (Mercury, Venus, Earth, Mars) and outer gas giants (Jupiter, Saturn, Uranus, Neptune).
  • A dwarf planet is similar to a planet but smaller; its gravity is not strong enough to clear its orbit of other objects.
  • Natural satellites (moons) orbit planets; artificial satellites (e.g., ISS) are man-made and orbit Earth.
  • Smaller bodies orbit larger ones: planets orbit the Sun, moons orbit planets.

The Solar System: the Sun, eight planets, natural and artificial satellites, and the asteroid belt

The Solar System: the Sun, eight planets, natural and artificial satellites, and the asteroid belt

Light Speed Calculations

  • Light travels at a constant speed of 3.0 × 10⁸ m/s in a vacuum.
  • Objects in the Solar System are visible because they reflect sunlight; light takes time to travel these large distances.
  • Light from the Sun takes about 8 minutes to reach Earth, and about 5 hours to reach the outer Solar System.
  • The time for light to travel a distance is calculated using: time = distance / speed of light.
  • Example: Light from Sun to Mercury (radius 5.8 × 10¹⁰ m) takes 193 s (about 3 minutes).

Gravitational Field Strength

  • Orbital motion is caused by the gravitational force of attraction between two bodies.
  • Gravitational force acts towards the centre of the larger body and keeps the orbiting body in a circular path.
  • The Sun's gravitational attraction keeps planets in orbit; the force is directed from the planet to the Sun's centre.
  • As distance from the Sun increases, the Sun's gravitational field strength decreases.
  • For a circular orbit, the centripetal force is provided by the Sun's gravitational attraction.
  • The further a planet is from the Sun: the smaller its orbital speed and the longer its orbital period.

The Sun's gravitational force of attraction keeps the Earth in orbit around the Sun

The Sun's gravitational force of attraction keeps the Earth in orbit around the Sun

Orbital Speed Equation

  • For a circular orbit, the distance travelled in one orbit is the circumference: 2πr.
  • The average orbital speed is given by: v = 2πr / T, where r is orbital radius and T is orbital period.
  • Orbital period is the time taken to complete one orbit.
  • The orbital radius r is measured from the centre of the body being orbited (e.g., from the Sun's centre for a planet).
  • If given height above a planet's surface, add the planet's radius to get the orbital radius.
  • Example: Hubble telescope at 560 km above Earth (Earth radius 6400 km) orbits in 96 min; its orbital speed is 7590 m/s.

Orbital radius is measured from the centre of mass of the body being orbited: r = R + h

Orbital radius is measured from the centre of mass of the body being orbited: r = R + h

Orbital Data and Trends

  • Mercury: orbital radius 57.9 million km, orbital speed 47.9 km/s, period 88 days.
  • Earth: orbital radius 149.6 million km, orbital speed 29.8 km/s, period 365 days.
  • Neptune: orbital radius 4495.1 million km, orbital speed 5.4 km/s, period 165 years.
  • The closest planets to the Sun have the fastest orbital speeds and shortest periods; the furthest have the slowest speeds and longest periods.

The closest planets to the Sun have the fastest orbital speeds, and the furthest have the slowest

The closest planets to the Sun have the fastest orbital speeds, and the furthest have the slowest

ஸ்லைடுகள்

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பயிற்சி கேள்விகள்

இலவச முன்னோட்டம் — 47-இல் 8 கேள்விகள். அனைத்தையும் பார்க்க பதிவு செய்யவும்.
  1. 1.What is the name of the star at the centre of the Solar System?

    Easy
    • AThe Sun
    • BEarth
    • CMercury
    • DThe Moon
  2. 2.How many planets are there in the Solar System?

    Easy
    • A7
    • B8
    • C9
    • D10
  3. 3.Arrange the following planets in order of increasing distance from the Sun.

    Easy
    • Earth
    • Jupiter
    • Mercury
    • Neptune
    • Saturn
    • Uranus
  4. 4.The Moon is a natural satellite of the Earth.

    Easy

    True or false?

  5. 5.Artificial satellites are natural objects that orbit planets.

    Easy

    True or false?

  6. 6.Complete the sentence:

    Easy

    The gravitational field around a ____ is strong enough to pull in nearby objects, but that around a dwarf planet is not.

  7. 7.State one difference between a planet and a dwarf planet.

    Medium
  8. 8.The radius of Mercury's orbit around the Sun is 5.8 × 1010 m. The speed of light is 3.0 × 108 m/s. Calculate the time taken for light from the Sun to reach Mercury. Give your answer in seconds.

    Medium
    • A231
    • B174
    • C193
    • D212

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இந்த தலைப்பிற்கான ஒவ்வொரு கேள்வியையும், ஸ்லைடுகளையும், ஃப்ளாஷ் கார்டுகளையும் மற்றும் திருப்புதல் குறிப்புகளையும் பார்க்க இலவச கணக்கை உருவாக்கவும்.

முந்தைய தேர்வுகள்

இந்த தலைப்பிற்கான முந்தைய தேர்வு பயிற்சி விரைவில் வருகிறது.
விரைவில் வருகிறது