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Related Concept Videos

Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
Biological Effects of Radiation02:59

Biological Effects of Radiation

All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they produce ions...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Real-World Applications of Space Curves01:29

Real-World Applications of Space Curves

Modern aerospace navigation depends on the accurate prediction of motion in three-dimensional space. In defense applications, radar systems continuously track both interceptors and moving aerial targets to find whether their flight paths will result in a collision. These motions are modeled mathematically as space curves, which represent paths that change continuously with time. Each object’s position is described by a vector function that specifies its location in terms of time-dependent...

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Related Experiment Video

Updated: Jun 24, 2026

Exploring the Effects of Spaceflight on Mouse Physiology using the Open Access NASA GeneLab Platform
11:08

Exploring the Effects of Spaceflight on Mouse Physiology using the Open Access NASA GeneLab Platform

Published on: January 13, 2019

Advancing space radiation risk assessment for deep space missions.

Satoshi Kodaira1, Teruaki Konishi1, Floriane Poignant2

  • 1Institute for Radiological Science, National Institutes for Quantum Science and Technology (QST), Chiba, Japan.

Life Sciences in Space Research
|June 22, 2026
PubMed
Summary

Space radiation risk assessment needs improved quality factors (Q) beyond current ground-based models. New methods incorporating track structure and biological responses are crucial for accurate deep space dosimetry.

Area of Science:

  • Space radiation physics and biology
  • Radiological protection
  • Dosimetry
Keywords:
Heavy ionsHigh LETIn vivo modelsInter-/Intra-cellular responseLow dose and Low dose rate effectMicrodosimetryQRBE

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Background:

  • Current space radiation risk assessment uses the quality factor (Q) defined by the International Commission on Radiological Protection (ICRP) Publication 60.
  • This Q-LET relationship, established for terrestrial dosimetry, may not accurately reflect the complexities of space radiation environments.
  • Accurate dose assessment is vital for astronaut safety during long-duration space missions.