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Related Concept Videos

Mutations01:35

Mutations

Mutations are changes in the sequence of DNA. These changes can occur spontaneously or they can be induced by exposure to environmental factors. Mutations can be characterized in a number of different ways: whether and how they alter the amino acid sequence of the protein, whether they occur over a small or large area of DNA, and whether they occur in somatic cells or germline cells.
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Mutations01:39

Mutations

Overview
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
X-ray Imaging01:24

X-ray Imaging

German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...
Role of Skin in Vitamin D Synthesis01:23

Role of Skin in Vitamin D Synthesis

The skin plays a crucial role in the synthesis of vitamin D, a vital nutrient for various physiological processes in the body. Vitamin D is unique because it can be synthesized in the skin through a series of chemical reactions triggered by exposure to ultraviolet B (UVB) radiation from sunlight.
The solar UV B rays (290-315 nm) are absorbed by the skin, and 7-dehydrocholesterol (provitamin D3) photolyzes it to previtamin D3, which undergoes a rapid transformation to vitamin D3(cholecalciferol).
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...

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Related Experiment Video

Updated: May 10, 2026

Studying Chronic Exposure of Mice to Ultraviolet B Radiation
03:20

Studying Chronic Exposure of Mice to Ultraviolet B Radiation

Published on: August 19, 2025

UV radiation and the skin.

John D'Orazio1, Stuart Jarrett, Alexandra Amaro-Ortiz

  • 1Graduate Center for Toxicology and the Departments of Pediatrics, Biomedical and Molecular Pharmacology and Physiology, Markey Cancer Center, University of Kentucky College of Medicine, 800 Rose Street, Lexington, KY 40536, USA. jdorazio@uky.edu.

International Journal of Molecular Sciences
|June 11, 2013
PubMed
Summary
This summary is machine-generated.

Ultraviolet (UV) radiation is a complete carcinogen, increasing skin cancer risk. Understanding UV

Related Experiment Videos

Last Updated: May 10, 2026

Studying Chronic Exposure of Mice to Ultraviolet B Radiation
03:20

Studying Chronic Exposure of Mice to Ultraviolet B Radiation

Published on: August 19, 2025

Area of Science:

  • Dermatology
  • Molecular Biology
  • Genetics
  • Oncology

Background:

  • Ultraviolet (UV) radiation is a complete carcinogen, acting as both a mutagen and a tumor promoter.
  • UV exposure is a primary modifiable risk factor for skin cancer and other skin disorders.
  • UV radiation has dual effects, benefiting health through vitamin D synthesis but posing risks like skin aging and malignancy.

Purpose of the Study:

  • To investigate the molecular mechanisms underlying UV-induced skin damage and cancer.
  • To explore the role of epidermal melanization and the melanocortin 1 receptor (MC1R) in UV protection and genome maintenance.
  • To develop novel UV-protective strategies based on a comprehensive understanding of UV radiation's molecular effects.

Main Methods:

  • Epidemiological and molecular analyses linking UV exposure to skin cancer.
  • Investigation of genetic factors, specifically melanocortin 1 receptor (MC1R) gene polymorphisms.
  • Focus on epidermal melanization processes and MC1R's role in genome maintenance following UV exposure.

Main Results:

  • UV radiation is epidemiologically and molecularly associated with basal cell carcinoma, squamous cell carcinoma, and malignant melanoma.
  • MC1R gene polymorphisms are correlated with skin type, UV sensitivity, and increased cancer risk.
  • Detailed understanding of molecular events post-UV exposure is crucial for developing protective measures.

Conclusions:

  • UV radiation poses significant risks for skin cancer and premature aging.
  • The MC1R gene plays a critical role in modulating UV sensitivity and cancer risk.
  • Further research into UV-induced molecular pathways, particularly melanization and MC1R function, is essential for advancing UV protection strategies.