Solar System Explained — Planets, Sun, Dwarf Planets, Asteroids, and Facts

Solar System — Planets, Sun, and Celestial Bodies Explained
Target Towards • Updated 2025

Solar System — Planets, Sun, and Celestial Bodies Explained

A complete and original study guide for students. Learn the Sun, each planet in detail with quick facts tables, dwarf planets, asteroids, meteors, comets, important space missions, and exam tips in clear English.

Introduction

The Solar System is the Sun together with all objects that orbit it under gravity. These objects include eight major planets, their moons, dwarf planets, a large number of asteroids, comets, and dust. The Solar System lies in the Milky Way galaxy. The Sun contains nearly all of the system’s mass, and its gravity keeps planets on steady paths.

This guide explains each major part in a clear, study-friendly format. Each planet section includes a short description followed by a mini-table of key facts. Use the tables for quick revision and the paragraphs for deeper understanding.

The Sun — Structure & Role

The Sun is a medium-sized star and the primary source of light and heat for the Solar System. It is mainly composed of hydrogen and helium. Energy is produced in the Sun’s core by nuclear fusion, where hydrogen nuclei combine to form helium and release a huge amount of energy as light and heat.

Sun: Explanatory details

Core: The Sun’s core is the hottest region where fusion occurs. Temperatures reach about 15 million °C. Fusion produces photons and particles that slowly travel outward.

Radiation and convection zones: Energy from the core moves outward through the radiation zone and then the convective zone. In the convective zone rising and falling plasma transports energy to the surface.

Photosphere, Chromosphere, Corona: The photosphere is the visible “surface” we see. Above it lie the chromosphere and the corona. The corona forms the Sun’s outer atmosphere and is visible during a total solar eclipse.

Magnetic activity: The Sun has magnetic fields that drive sunspots, solar flares, and coronal mass ejections. These events can affect satellites and communications on Earth and create auroras near the poles.

FeatureDetails
Main componentsHydrogen (~75%), Helium (~24%)
Core temperature≈ 15 million °C
Visible surfacePhotosphere ≈ 5,500–6,000 °C
RolePrimary energy source; central gravitational body

Mercury — The Small Fast Planet

Mercury is the closest planet to the Sun and the smallest of the eight major planets. It has a very thin or almost no atmosphere which means temperatures change widely between day and night. Its surface is heavily cratered and resembles the Moon.

Mercury moves quickly along its orbit and has a short year. It lacks significant atmosphere to retain heat or support weather.

PropertyMercury
TypeInner (terrestrial) planet
Orbital period (year)≈ 88 Earth days
Rotation (day)≈ 58.6 Earth days (slow rotation)
Major moonsNone
AtmosphereExtremely thin — almost vacuum (trace gases)
Surface / compositionRocky, heavy cratering, iron-rich core
Special featuresVery large iron core; extreme temperature swings

Venus — Earth’s Twin with a Hostile Climate

Venus is similar to Earth in size and mass, which is why it is called Earth’s twin. But its thick atmosphere of carbon dioxide creates an intense greenhouse effect. Surface temperatures are extremely high — hot enough to melt lead. Winds and clouds of sulfuric acid make the environment hostile to life as we know it.

Venus rotates slowly and in the opposite direction to most planets. One day on Venus (one full rotation) is longer than one Venus year (one orbit around the Sun).

PropertyVenus
TypeInner (terrestrial) planet
Orbital period (year)≈ 225 Earth days
Rotation (day)≈ 243 Earth days (retrograde rotation)
Major moonsNone
AtmosphereThick CO₂ with clouds of sulfuric acid
Surface / compositionRocky, volcanic plains, few large highlands
Special featuresStrong greenhouse effect; brightest planet in sky

Earth — Our Home Planet

Earth is the only known planet that supports life. It has abundant liquid water on its surface, a protective atmosphere with oxygen, and moderate temperatures that support ecosystems. The atmosphere and magnetic field protect life from harmful solar radiation.

Earth’s tilt of about 23.5° causes seasons. Its single natural satellite, the Moon, affects tides and stabilizes Earth’s rotation over long timescales.

PropertyEarth
TypeInner (terrestrial) planet
Orbital period (year)≈ 365.25 days
Rotation (day)≈ 24 hours
Major moonsMoon (Luna)
AtmosphereNitrogen (≈78%), Oxygen (≈21%), trace gases
Surface / compositionRocky crust, liquid water oceans, continents
Special featuresOnly known life-bearing planet; protective magnetosphere

Important points about Earth (quick)

  • Oceans cover about 71% of Earth’s surface.
  • Atmospheric layers block harmful solar rays and maintain climate.
  • Tides are caused mainly by the Moon’s gravity.
  • Earth’s rotation and orbit cause day/night and seasons.

Mars — The Red Planet

Mars appears red due to iron oxide (rust) in its soil. It has the tallest volcano in the Solar System (Olympus Mons) and large valleys such as Valles Marineris. Past water flow is evident in dry riverbeds and mineral deposits — this makes Mars a key target for searching past life.

Mars has two small moons — Phobos and Deimos — and a thin atmosphere mostly of carbon dioxide. Temperatures are cold, and dust storms can cover the planet.

PropertyMars
TypeInner (terrestrial) planet
Orbital period (year)≈ 687 Earth days
Rotation (day)≈ 24 hours 37 minutes
Major moonsPhobos, Deimos
AtmosphereThin CO₂ atmosphere with trace gases
Surface / compositionRocky, iron-rich soil, volcanoes, canyons
Special featuresEvidence of past water; Olympus Mons; interest for human exploration

Jupiter — The Giant Planet

Jupiter is the largest planet in the Solar System. It is mostly hydrogen and helium and has no solid surface like Earth. Its thick atmosphere shows colorful cloud bands and the famous Great Red Spot — a massive storm that has lasted for centuries.

Jupiter has many moons; several are large and important for study. Its strong gravity influences the asteroid belt and helps protect inner planets by capturing or deflecting comets and asteroids.

PropertyJupiter
TypeOuter (gas giant)
Orbital period (year)≈ 11.86 Earth years
Rotation (day)≈ 9 hours 50 minutes (fast rotation)
Major moonsIo, Europa, Ganymede, Callisto (Galilean moons)
AtmosphereHydrogen and helium with traces of methane, ammonia
Surface / compositionNo solid surface; dense atmosphere over deep metallic hydrogen
Special featuresLargest planet; strong magnetic field; many moons; Great Red Spot

Saturn — The Ringed Planet

Saturn is famous for its extensive ring system made of ice and rock particles. Like Jupiter, Saturn is mostly hydrogen and helium and lacks a true solid surface. Saturn has many moons, including Titan, which has a dense atmosphere and liquid hydrocarbon lakes.

PropertySaturn
TypeOuter (gas giant)
Orbital period (year)≈ 29.5 Earth years
Rotation (day)≈ 10 hours 30 minutes
Major moonsTitan, Rhea, Enceladus, Iapetus (selected)
AtmosphereHydrogen and helium with trace gases
Surface / compositionNo solid surface; interior of hydrogen and helium
Special featuresExtensive ring system; Titan’s atmosphere and Enceladus’ geysers

Uranus — The Tilted Ice Giant

Uranus is an ice giant with a blue-green color from methane gas in its atmosphere. A unique feature is its extreme axial tilt — it rotates on its side, so its poles point nearly toward the Sun during parts of its orbit. Uranus has faint rings and many small moons.

PropertyUranus
TypeOuter (ice giant)
Orbital period (year)≈ 84 Earth years
Rotation (day)≈ 17 hours
Major moonsTitania, Oberon, Umbriel, Ariel, Miranda (selected)
AtmosphereHydrogen, helium, methane (gives blue-green color)
Surface / compositionIce-rich interior; small rocky core
Special featuresExtreme axial tilt (~98°); faint rings

Neptune — The Windy Ice Giant

Neptune is the outermost of the eight planets. It is an ice giant with strong winds and large storms. Its deep blue color comes from methane and other components in its atmosphere. Neptune has several moons and faint rings.

PropertyNeptune
TypeOuter (ice giant)
Orbital period (year)≈ 165 Earth years
Rotation (day)≈ 16 hours
Major moonsTriton (largest), Nereid (selected)
AtmosphereHydrogen, helium, methane
Surface / compositionIce-rich interior around a rocky core
Special featuresStrongest winds in the Solar System; Triton is geologically active

Dwarf Planets

Dwarf planets are bodies that orbit the Sun and are round in shape but have not cleared their orbital path of other debris. The most well-known dwarf planets include Pluto, Ceres, Eris, Haumea, Makemake. Ceres is found in the asteroid belt, while others are in the Kuiper Belt beyond Neptune.

Key points about dwarf planets:
  • Dwarf planets follow the Sun but share their orbital zones with other objects.
  • Pluto was reclassified as a dwarf planet in 2006 by the IAU.
  • Ceres is the only dwarf planet located in the inner Solar System (asteroid belt).

Asteroids & The Asteroid Belt

Asteroids are rocky bodies that orbit the Sun. Most are found in the Asteroid Belt between Mars and Jupiter. They are remnants from the early Solar System that never formed into a planet, mainly because Jupiter’s gravity disturbed their growth.

Asteroids range from tiny pebbles to objects hundreds of kilometers across (for example, Vesta and Ceres). Some asteroids cross Earth’s orbit and can be potentially hazardous if on a collision course.

Meteors, Meteorites & Bolides

A meteor is the bright streak we see when a small rock or dust particle enters Earth’s atmosphere and burns up from friction — commonly called a shooting star. If the object survives the fall and lands on Earth, it is a meteorite.

Large impacts can form craters. Example: Lonar Lake in India is an impact crater formed by a meteorite.

Comets

Comets are icy bodies from the distant reaches of the Solar System. When a comet approaches the Sun, its ices vaporize and produce a glowing head (coma) and a long tail that points away from the Sun. Comets come from regions such as the Kuiper Belt and the Oort Cloud.

Well-known comets include Halley’s Comet, which returns approximately every 76 years.

Key Space Missions That Changed Our Knowledge

Robotic space missions have provided most of our detailed knowledge about planets and small bodies. Below are important missions that are essential to know for study:

  • Voyager 1 & 2: Explored outer planets and continue to send data from interstellar space.
  • Curiosity & Perseverance: Mars rovers studying geology and signs of past life.
  • New Horizons: Flew past Pluto and explored Kuiper Belt objects.
  • Cassini: Explored Saturn and its moons, discovered active plumes on Enceladus.
  • Parker Solar Probe: Studying the Sun’s outer corona up close.

Important Facts & Exam Tips

Key facts to remember
  • The Sun contains about 99.8% of the Solar System’s mass.
  • There are eight major planets: Mercury → Venus → Earth → Mars → Jupiter → Saturn → Uranus → Neptune.
  • Pluto is a dwarf planet — classification changed in 2006.
  • Asteroid Belt lies between Mars and Jupiter.
  • Comets often come from the Kuiper Belt and the Oort Cloud.
Exam tips
  • Use mnemonics for planet order: My Very Educated Mother Just Served Us Noodles.
  • Remember the difference: planet (clears orbit) vs dwarf planet (does not clear orbit).
  • For quick answers, memorize each planet’s orbit (approximate year), rotation period, and one special feature.
  • Practice short definitions: photosphere, corona, asteroid belt, comet, meteorite.

Notes (PDF) — Hindi

⤓ Solar System Notes (PDF)

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