- (a) Tycho Brahe
- (b) Nicolaus Copernicus
- (c) Ptolemy
- (d) Archimedes
Answer:
(b) Nicolaus Copernicus
- (a) Mercury
- (b) Saturn
- (c) Uranus
- (d) Neptune
Answer:
(a) Mercury
- (a) meteor
- (b) star
- (c) planet
- (d) asteroid
Answer:
(d) asteroid
Ceres is also classified as a dwarf planet.
- (a) 4
- (b) 5
- (c) 2
- (d) 3
Answer:
(a) 4
Using Kepler’s Third Law:
- (a) 13.7 billion years ago
- (b) 15 million years ago
- (c) 15 billion years ago
- (d) 20 million years ago
Answer:
(a) 13.7 billion years ago
Modern estimate is approximately 13.8 billion years.
- Speed of the Sun around the Milky Way is about 250 km/s.
- Rotational period of the Sun near poles is about 36 days.
- India’s first satellite was Aryabhata.
- Kepler’s third law is also called Law of Harmonics.
- Number of planets in Solar System is 8.
If false, correct the statement.
Answer: True
This statement is false. Halley's comet does not appear after nearly 67 hours. The correct statement is that Halley's comet appears approximately every 76 years. This periodic comet is one of the most famous comets visible from Earth and follows a regular orbital path around the Sun. It was last visible in 1986 and is expected to return in 2061. The comet is named after English astronomer Edmond Halley, who predicted its periodic return based on observations of comets in previous centuries.
This statement is false. Satellites nearer to Earth require greater orbital velocity, not lesser. The orbital velocity of a satellite depends on its distance from Earth's center. Satellites in lower orbits, closer to Earth, must travel faster to maintain their circular orbit and counteract Earth's stronger gravitational pull at that distance. Conversely, satellites in higher orbits, farther from Earth, experience weaker gravitational force and therefore require lower orbital velocities. This relationship is described by the formula for orbital velocity, which shows that velocity is inversely proportional to the square root of the orbital radius.
This statement is true. Mars is called the Red Planet because its surface appears reddish in color. This reddish appearance is due to the presence of iron oxide, commonly known as rust, on the Martian surface. The iron oxide gives Mars its distinctive red hue, which is visible even from Earth when observed through telescopes. This characteristic color is one of the most recognizable features of Mars and is the reason it has earned the nickname the Red Planet.
Answer:
The Sun and all celestial bodies revolving around it together form the Solar System.
It includes:
- planets
- satellites
- asteroids
- comets
- meteors
Orbital velocity is defined as the horizontal velocity required for a satellite to revolve around Earth in a stable circular orbit. It is the minimum velocity at which a satellite must travel tangentially to the Earth's surface so that it falls toward Earth at the same rate as Earth's surface curves away from it. At this velocity, the gravitational force provides exactly the centripetal force needed to keep the satellite in circular motion. The orbital velocity depends on the mass of Earth and the orbital radius of the satellite. For a satellite orbiting close to Earth's surface, the orbital velocity is approximately 7.9 km/s or 28,400 km/h.
Answer:
Time taken by satellite to complete one revolution around Earth is called orbital period.
Answer:
A body revolving around a planet is called satellite.
Types:
- Natural satellites
- Artificial (man-made) satellites
Answer:
Inner planets are planets close to Sun.
They are:
- Mercury
- Venus
- Earth
- Mars
Features:
- Rocky planets
- High density
- Smaller size
They are also called:
Terrestrial Planets
Answer:
- Comets are made of dust, rock and ice.
- They revolve around Sun in highly elliptical orbits.
- On approaching Sun, they form glowing head and tail.
- Tail always points away from Sun.
Example:
Halley’s Comet
First Law – Law of Ellipses
Planets revolve around Sun in elliptical orbits.
Sun lies at one focus.
Second Law – Law of Equal Areas
Line joining planet and Sun sweeps equal areas in equal intervals of time.
Third Law – Law of Harmonics
Square of orbital period is proportional to cube of semi-major axis.
Answer:
- Suitable distance from Sun
- Suitable temperature
- Presence of water
- Atmosphere
- Ozone layer
# Mercury
- Nearest planet to Sun
- Rocky planet
- Fastest revolution
# Venus
- Hottest planet
- Similar size to Earth
- Rotates opposite direction
# Earth
- Only known life-supporting planet
- Blue appearance due to water
- Revolution period:
# Mars
- Red planet
- Two small moons
# Jupiter
- Largest planet
- Gas giant
- Has Great Red Spot
# Saturn
- Famous for rings
- Gas giant
# Uranus
- Rotates on its side
- Cold gas giant
# Neptune
- Windiest planet
- Has moon Triton
ISS = International Space Station
Benefits:
- Water purification technology
- Medical advancements
- Robotic surgery techniques
- Vaccine development
- Cancer research
Definition
Minimum horizontal velocity needed to keep satellite in orbit.
Important Points
- Depends on altitude
- Nearer satellites require greater speed
Formula
Where:
- (G) = gravitational constant
- (M) = mass of Earth
- (R) = radius of Earth
- (h) = orbital height
Geostationary Orbit
Satellite appears fixed relative to Earth.
Orbital period:
Answer:
Colour depends on temperature.
- Hot stars → blue/white
- Cooler stars → orange/red
A satellite is maintained in a circular orbit around Earth through the balance between its horizontal velocity and Earth's gravitational force. When a satellite is launched, it is given a high horizontal velocity in a direction tangent to Earth's surface. Earth's gravity continuously pulls the satellite toward Earth's center, providing the centripetal force necessary for circular motion. The satellite falls toward Earth, but because of its high horizontal velocity, it keeps missing Earth and instead follows a curved path around it. This balance between the satellite's inertia, which tends to make it move in a straight line, and Earth's gravitational pull, which pulls it toward the center, results in a stable circular orbit. If the velocity were too low, the satellite would fall back to Earth; if too high, it would escape Earth's gravitational field.
Satellites are called geostationary because they revolve around Earth in the equatorial plane in the same direction as Earth's rotation, with an orbital period of approximately 24 hours, which matches Earth's rotational period. This synchronization causes the satellite to remain fixed above the same point on Earth's surface at all times. A geostationary orbit is located at a height of about 36,000 km above Earth's surface. These satellites are extremely useful for telecommunications, weather monitoring, and broadcasting because their stationary position relative to Earth allows continuous coverage of a fixed geographical area without the need for tracking equipment.
Answer:
The person’s mass remains 60 kg, but weight depends on gravity.
So, the person’s weight on the Sun is about 16,440 N, equal to the weight of a 1680 kg mass on Earth. The person’s mass remains 60 kg.
Given:
Using orbital velocity formula:
Answer:
or
Given:
Using orbital period relation:
Answer:
Poster on Astronomers
Aim:
To learn contributions of astronomers.
Examples:
- Copernicus
- Galileo
- Kepler
- Newton
Observe Constellations
Observation:
Groups of stars form recognizable patterns.
Examples:
- Orion
- Ursa Major
Observe Planets
Observation:
Some planets visible to naked eye:
- Mercury
- Venus
- Mars
- Jupiter
- Saturn
Indian Satellites
Example List:
| Satellite | Purpose |
|---|---|
| Aryabhata | Scientific research |
| INSAT | Communication |
| IRS | Remote sensing |
| Chandrayaan | Moon mission |
| Mangalyaan | Mars mission |
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