The Solar System: Planets, Definitions, and Classifications

Planets and dwarf planets of our solar system (Milky Way)

What are Planets?

Planets are solid celestial bodies that revolve around a star, such as the Sun, in elliptical orbits. Composed of rock and metal, they do not emit their own light but shine by reflecting sunlight. Unlike stars, planets are closer to Earth and do not twinkle at night. They move from west to east around the Sun, causing their positions to change daily. Planets are much smaller than the Sun or stars. There are eight major planets in our Solar System.

Planets and dwarf planets of our solar system (Milky Way)

List of Planets in the Solar System (in order of increasing distance from the Sun):

  1. Mercury (Budha): Nearest to the Sun.
  2. Venus (Shukra)
  3. Earth (Prithvi)
  4. Mars (Mangal)
  5. Jupiter (Brihaspati): The largest planet.
  6. Saturn (Shani)
  7. Uranus (Arun)
  8. Neptune (Varun)

IAU Definition of a Planet

In 2006, the International Astronomical Union (IAU) defined a planet in the Solar System as a celestial body that:

  • Is in orbit around the Sun,
  • Has sufficient mass to assume hydrostatic equilibrium (a nearly round shape),
  • Has “cleared the neighborhood” around its orbit, making it the dominant gravitational body in its orbit.

A celestial body that meets the first two criteria but not the third is classified as a dwarf planet. For example, Pluto is considered a dwarf planet because it has not cleared its orbit.

READ ALSO  Endogenetic Forces and Their Impact on Earth's Landforms

Classification of Planets

Terrestrial Planets

The four planets closest to the Sun—Mercury, Venus, Earth, and Mars—are known as terrestrial planets due to their Earth-like structure. Common features of terrestrial planets include:

  • Thin, rocky crusts
  • Mantles rich in iron and magnesium
  • Cores of heavy metals
  • Thin atmospheres
  • Few or no natural satellites
  • Varied terrains such as volcanoes, canyons, mountains, and craters

Jovian Planets

The planets beyond Mars—Jupiter, Saturn, Uranus, and Neptune—are called Jovian planets, as their structure resembles that of Jupiter. Common features of Jovian planets include:

  • Being gaseous bodies
  • Possessing ring systems
  • Having a large number of natural satellites
 SunMERC URYVEN USEAR THMO ONMA RSJUPIT ERSATU RNURAN USNEPT UNEPLUT O
Mass (1024k)1,988, 5000.334.875.970.07 30.6 42189856886.81020.013 1
Diameter (k m)1,392, 684487912,1 0412,7 56347 5679 2142,9 84120,5 3651,11 849,52 82390
Density (kg/ m3)1,4085427524 3551 4334 0393 31326687127116381830
Gravity (m/s 2) 3.78.99.81.63.723.198.7110.6
Escape Velocity (km/ s) 4.310.411.22.4559.535.521.323.51.1
Rotation Period (hour s) 1407. 6– 583 2.523.9655. 724. 69.910.7-17.216.1– 153.3
Length          of Day (hours) 4222. 6280 224708. 724. 79.910.717.216.1153.3
Distance from Sun (106 km) 57.9108. 2149. 60.38 4227 .9778.61433. 52872. 54495. 15870
Perihelion (1 06 km) 46107. 5147. 10.36 3206 .6740.5The Solar System: Planets, Definitions, and Classifications2741. 34444. 54435
Aphelion (10 6 km) 69.8108. 9152. 10.40 6249 .2The Solar System: Planets, Definitions, and Classifications1514. 53003. 64545. 77304. 3
Orbital Period (days) 88224. 7365. 227.3The Solar System: Planets, Definitions, and Classifications687433110,74 730,58 959,80 090,58 8
Orbital Velocity (km/ s) 47.93529.8124. 113.19.76.85.44.7
Orbital Inclination (d egrees) 73.405.11.91.32.50.81.817.2
Orbital Eccentricity 0.2050.00 70.01 70.05 50.0 940.0490.0570.0460.0110.244
Axial Tilt (degrees) 0.01177. 423.46.725. 23.126.797.828.3122.5
Mean Temperature  (C) 16746415-20-65-110-140-195-200-225
Surface Pressure (bar s) 092100.0 1Unkn ownUnkn ownUnkn ownUnkn own0
Number               of Moons 00102676227145
Ring System? NoNoNoNoNoYesYesYesYesNo
Global Magnetic Field? YesNoYesNoNoYesYesYesYesUnkn own
Reference = NASA

Responses