Comets are small celestial bodies made mainly of:
They revolve around the Sun and become highly visible when they approach the inner Solar System.
Comets generally revolve around the Sun in:
These orbits are characterized by two important points:
| Term | Meaning |
|---|---|
| Perihelion | Closest point to the Sun |
| Aphelion | Farthest point from the Sun |
Because of these elongated paths:
The orbital motion of comets is governed by:
A comet develops a tail when it comes close to the Sun.As the comet approaches the Sun:
This produces a glowing cloud around the nucleus called the:
The coma consists of:
Further interaction with:
results in the formation of the comet’s tail.
The tail always points away from the Sun because:
Thus, the tail direction depends on solar forces rather than the direction of comet movement.
| Feature | Description |
|---|---|
| Composition | Ionized gases |
| Shape | Straight |
| Direction | Directly away from the Sun |
| Cause | Solar wind |
The ion tail often appears bluish.
| Feature | Description |
|---|---|
| Composition | Fine solid particles |
| Shape | Curved |
| Cause | Solar radiation pressure |
The dust tail generally appears yellowish or white.
The solid central part of a comet is called the:
It mainly contains:
| Comet | Important Fact |
|---|---|
| Halley’s Comet | Visible roughly every 76 years |
| Hale-Bopp | One of the brightest modern comets |
| Comet NEOWISE | Became visible in 2020 |
| Feature | Comets | Asteroids |
|---|---|---|
| Composition | Ice and dust | Rocky/metallic |
| Tail Formation | Present | Usually absent |
| Orbit | Highly elliptical | Less elongated |
| Appearance Near Sun | Bright coma and tail develop | No tail |
Uranus is the:
It is one of the most unusual planets because of its:
Uranus was discovered in:
by astronomer:
It was the first planet discovered using a telescope.Initially, Herschel thought the object was:
before it was identified as a planet.
| Feature | Details |
|---|---|
| Position from Sun | Seventh planet |
| Diameter Rank | Third largest |
| Type | Ice Giant |
| Rotation Nature | Retrograde |
| Axial Tilt | About 98° |
Uranus rotates in an extremely unusual manner.Its axis of rotation is tilted by nearly:
This means:
Unlike other planets:
Thus:
Most planets:
However:
Both planets show:
This means they rotate opposite to the Sun’s rotational direction.
Retrograde rotation refers to:
Scientists have proposed multiple hypotheses to explain Uranus’s unusual tilt.
One major theory suggests that:
The impact may have:
This theory also explains:
Simulations conducted in 2011 suggested a different explanation.According to these studies:
These repeated impacts gradually tilted the planet to:
This multiple-impact theory gained support because:
Scientists argued that:
Another theory proposed in 2009 suggested that:
The gravitational pull of this moon may have gradually tilted Uranus onto its side.Later:
This process has been compared to:
Venus also displays:
Scientists believe Venus may similarly have experienced:
| Feature | Uranus |
|---|---|
| Planet Type | Ice Giant |
| Discovery Year | 1781 |
| Discoverer | William Herschel |
| Axial Tilt | ~98° |
| Rotation | Retrograde |
| Position from Sun | Seventh |
| Feature | Uranus | Venus |
|---|---|---|
| Rotation | Retrograde | Retrograde |
| Tilt | Extreme sideways tilt | Very small tilt |
| Main Hypothesis | Collisions/gravitational effects | Massive collision or atmospheric effects |
Uranus is among the most unique planets in the Solar System because of its extreme axial tilt and retrograde rotation. Various theories involving giant impacts, repeated collisions, and gravitational interaction with a former moon attempt to explain its unusual orientation. However, no single explanation has been definitively confirmed, making Uranus an important subject in planetary evolution studies.
Because of the:
different parts of Earth receive varying amounts of sunlight during the year.This gives rise to:
It is one of the two moments in a year when:
It is the second moment in the year when:
It occurs when:
It occurs when:
| Event | Date | Sun Overhead Position | Important Feature |
|---|---|---|---|
| Vernal Equinox | 21 March | Equator | Equal day and night; beginning of spring |
| Summer Solstice | 21 June | Tropic of Cancer | Longest day in Northern Hemisphere |
| Autumnal Equinox | 23 September | Equator | Equal day and night; beginning of autumn |
| Winter Solstice | 22 December | Tropic of Capricorn | Shortest day in Northern Hemisphere |