Sections View Full Chapter Figures Tables Videos Annotate Full Chapter Figures Tables Videos Supplementary Content +++ SKIN AGING ++ Intrinsic aging: natural or chronologic aging, influenced by genetics Begins in the mid-20s, but signs may not be visible for decades Collagen production and cell turnover slows Loss of subcutaneous fat and bone loss contribute to volume issues Extrinsic aging: caused by environmental factors Largest contributors are ultraviolet (UV) radiation (photoaging) and smoking Facial expressions, sleeping positions, nutrition, and airborne particles (pollution) are additive factors Solar elastosis or dermatoheliosis: term applied to the chronic inflammatory changes and degradation of elastin and collagen +++ OXIDATIVE STRESS (FREE RADICAL THEORY OF AGING) ++ Reactive oxygen species (ROS) derived from the environment and oxidative cell metabolism damage cellular components and lead to aging Mitochondria are the main endogenous source of ROS ROS activate signal transduction pathways including mitogen-activated protein kinases, c-jun N-terminal kinase (JNK), and extracellular signal related kinases, which upregulate the nuclear transcription factor activator protein 1 (AP-1) AP-1 activates matrix metalloproteinase (MMP) genes for MMP-1 (collagenase), MMP-3 (stromolysin), and MMP-9 (gelatinase) MMPs degrade collagen types I and III AP-1 inhibits transforming growth factor B (TGF-B), a profibrotic cytokine, and downregulates type II TGF-B receptors so cells cannot respond to TGF-B and less type I procollagen is produced Antioxidants such as vitamins A, C, and E, ubiquinone and glutathione may help to minimize ROS-induced damage All-trans-retinoic acid (tretinoin) acts like an antioxidant to inhibit the accumulation of c-jun protein, thereby preventing the formation of AP-1 and the upregulation of MMPs Tretinoin also induces TGF-B to enhance production of procollagen types I and III +++ Ultraviolet Radiation ++ UVA: 320 to 400 nm; largest contributor to Aging due to deeper penetration depth and ability to generate ROS UVA1: 340 to 400 nm (longest wavelength and deepest penetration of all ultraviolet light) UVA2: 320 to 340 nm UVB: 290 to 320 nm; Burning rays; absorbed by the epidermis, mainly causing damage to keratinocytes in the form of pyrimidine dimers Narrowband UVB: 311 to 312 nm UVC: 100 to 290 nm; has negligible effect on skin as nearly all is blocked by the atmosphere UVA rays make up 95% of UV radiation reaching the Earth's surface; however UVB rays are more intense Both contribute to skin cancer, photoaging (wrinkles, discoloration, telangiectasias), and ocular changes (cataracts, pterygium) UV radiation downregulates gene expression in types I and III procollagen in dermal fibroblasts UV radiation activates transcription factor nuclear factor κB (NF-κB), resulting in transcription of proinflammatory cytokines such as IL-1β, tumor necrosis factor α, IL-6, and IL-8. Proinflammatory cytokines bind receptors on the cell surface to further activate AP-1 and NF-κB, escalating the photoaging response Activation of MMP-1 and NF-κB are iron dependent mechanisms, so iron chelators such as kojic acid may be included in topical antiaging preparations +++ Telomeres and Aging ++ Telomeres form the ends of human chromosomes; defend the ends of chromosomes ... Your Access profile is currently affiliated with [InstitutionA] and is in the process of switching affiliations to [InstitutionB]. Please select how you would like to proceed. Keep the current affiliation with [InstitutionA] and continue with the Access profile sign in process Switch affiliation to [InstitutionB] and continue with the Access profile sign in process Get Free Access Through Your Institution Learn how to see if your library subscribes to McGraw Hill Medical products. Subscribe: Institutional or Individual Sign In Error: Incorrect UserName or Password Username Error: Please enter User Name Password Error: Please enter Password Sign in Forgot Password? Forgot Username? Sign in via OpenAthens Sign in via Shibboleth You already have access! Please proceed to your institution's subscription. Create a free profile for additional features.