Approval of Venus Mission Shukrayaan UPSC

Approval of Venus Mission Shukrayaan UPSC: The Indian government has approved ISRO’s Venus Orbiting Satellite mission, named “Shukrayaan.” Mission Shukrayan, or Venus Orbiter Mission (VOM), by the Department of Space. It will explore the atmosphere and surface of Venus and its interaction with the sun.

Approval of Venus Mission Shukrayaan UPSC

Aspect Details
Mission Name Shukrayaan-1
Launch Date Scheduled for 2028
Objective To explore Venus’s surface, atmosphere, and geological features.

  • Atmospheric Studies: Analyze the composition of Venus’s thick, carbon dioxide-rich atmosphere. Study the extreme greenhouse effect and its impact on the planet’s climate.
  • Surface Mapping: Utilize advanced radar technology to map the planet’s surface, revealing hidden geological features.
  • Ionospheric Studies: Explore the upper atmosphere of Venus, including the ionosphere, to understand its interaction with solar radiation and the solar wind.
Launch Vehicle GSLV Mk II
Key Instruments Synthetic Aperture Radar, Infrared and Ultraviolet Imaging Devices
Focus Areas Weather patterns, geological activity, atmospheric composition
Significance The first Indian mission to Venus aims to provide a global dataset for future science missions
Challenges Extreme temperatures, dense cloud cover of carbon dioxide and sulfuric acid
Potential Discoveries Signs of volcanic formations, possible microbial life in upper atmospheric layers
Scientific Payload:
  • Synthetic Aperture Radar (SAR): To penetrate the thick clouds and map the surface features.
  • Infrared Spectrometer: To study the composition of the atmosphere and surface.
  • Ultraviolet Spectrometer: To analyze the upper atmosphere and ionosphere.

Facts About Venus

Here are the key facts of Venus:

Aspect Details
Planetary Position 2nd planet from the Sun
Diameter About 12,104 km (7,521 miles)
Day Length 243 Earth days (longest day of any planet in the Solar System)
Year Length 225 Earth days
Surface Temperature Average temperature of around 467°C (872°F)
Atmosphere Thick clouds of carbon dioxide and sulfuric acid
Atmospheric Pressure 92 times that of Earth’s
Surface Features Volcanic plains, mountains, and craters
Magnetic Field Weak compared to Earth
Rotation Direction Retrograde (rotates in the opposite direction to most planets)
Moons None
Exploration Missions Mariner 2, Venera series, Magellan, Akatsuki
  • Venus, the second planet from the Sun.
  • It is often called Earth’s twin but is a harsh and hellish world.
  • Venus’s atmosphere is incredibly dense, composed primarily of carbon dioxide. This dense atmosphere traps heat from the sun, creating the runaway greenhouse effect.
  • Venus is the hottest planet in the solar system.
  • Several space missions, including Mariner 2, Venera, and Magellan, have studied Venus, providing valuable insights into its atmosphere, surface, and geology.
  • Future missions, such as NASA’s VERITAS and DAVINCI+, aim to further explore Venus.
  • Venus is named after the goddess of love.
  • Venus rotates on its axis in the opposite direction to most other planets, a phenomenon known as retrograde rotation. This means that the sun rises in the west and sets in the east on Venus.

Past and future Missions To Venus

  • Past missions:  Mariner 2 (USA, 1962),  Venus Express (ESA), Magellan (NASA),  Akatsuki (Japan), etc.
  • Future missions: Venus life finder mission (Rocket Lab and MIT), DAVINCI and VERITAS (NASA), EnVision (ESA)
Scroll to Top