Risks of Manned Space Exploration (SQA National 5 Physics): Revision Note

Exam code: X857 75

Katie M

Written by: Katie M

Reviewed by: Leander Oates

Updated on

Risks of manned space exploration

  • Space exploration poses significant risks for astronauts due to the extreme environments they are subjected to

  • Some of these risks include:

    • fuel load on take-off

    • potential exposure to radiation

    • pressure differential

    • re-entry through an atmosphere

Fuel load on take-off

  • Launching a spacecraft from Earth requires a large thrust to overcome the Earth's gravitational pull

  • To achieve take-off and maintain enough thrust to reach space, rockets must burn a large quantity of fuel

    • At launch, the fuel makes up around 90% of the total mass of the spacecraft

  • Risk to astronauts:

    • The rocket fuel is highly volatile

    • Therefore, a small spark or mechanical failure could ignite the fuel and cause an explosion

The space shuttle Challenger lifts off by expelling plumes of hot gas
In 1986, the space shuttle Challenger exploded 73 seconds after lift-off due to a mechanical fault

Photo credit: NASA (opens in a new tab)

Exposure to radiation

  • Outside Earth’s protective atmosphere and magnetic field, astronauts are exposed to:

    • cosmic rays (high-energy particles from space)

    • solar radiation (charged particles from the Sun)

  • Risk to astronauts:

    • Ionising radiation can damage cells and cause DNA to mutate

    • Therefore, astronauts are at an increased risk of developing cancer or, in severe cases, acute radiation sickness

Effect of radiation on a living cell

Ionising radiation entering a human cell nucleus, breaking DNA and potentially causing a mutation.
Ionising radiation from cosmic radiation and solar flares can cause damage to DNA. Sometimes the cell can successfully repair the DNA, but incorrect repairs can cause a mutation

Pressure differential

  • Inside a spacecraft or spacesuit, astronauts require the internal pressure to be equal to atmospheric pressure (the pressure at sea level on Earth)

  • Outside, in space, the external pressure is almost zero

    • This creates a large pressure differential, i.e. the difference between internal and external pressure

  • Risk to astronauts:

    • The pressure difference produces a large outward force on the spacecraft

    • If a breach (rupture) occurs, e.g. due to impact from space debris, in the spacecraft's hull or in a spacesuit (during a spacewalk), air would rush out very quickly

Re-entry into the atmosphere

  • When a spacecraft returns to Earth, it enters the atmosphere at a very high velocity

  • Friction between the spacecraft and the air generates heat energy, which causes the temperature to increase significantly

    • This is because the work done by friction transforms kinetic energy into heat

  • Risk to astronauts:

    • If a spacecraft is not protected from the heat, it could suffer a catastrophic failure or 'burn up' in the atmosphere

Heat shielding

  • To protect the astronauts and the spacecraft, heat shielding is required

  • Heat shields are made from insulating tiles with a high specific heat capacity and a high melting point, which allows them to

    • absorb a large amount of heat energy

    • radiate the heat energy back into the atmosphere

  • Heat shields are also coated with a substance with a high specific latent heat, which allows it to

    • absorb a large amount of heat energy without raising the temperature of the spacecraft

    • carry the energy away into the atmosphere as it melts (vaporises)

Heat shielding on the space shuttle

Spacecraft re-entering Earth's atmosphere, glowing from friction heat. Insulating tiles on the underside act as a heat shield, close-up shown.
The tiles used as a heat shield are extremely poor conductors of heat, so they are able to withstand the extreme heat produced by re-entry into the atmosphere

Examiner Tips and Tricks

Exam questions are sometimes asked about the re-entry of spacecraft, which may involve the following calculations:

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Katie M

Author: Katie M

Expertise: Physics Content Creator

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.

Leander Oates

Reviewer: Leander Oates

Expertise: Physics Content Creator

Leander graduated with First-class honours in Science and Education from Sheffield Hallam University. She won the prestigious Lord Robert Winston Solomon Lipson Prize in recognition of her dedication to science and teaching excellence. After teaching and tutoring both science and maths students, Leander now brings this passion for helping young people reach their potential to her work at SME.