中国自主创新企业
3A质量服务诚信企业
国家级科技企业孵化器
重点培育项目
咨询热线:400-8338-918
  • 首页
  • 当前位置:首页 > 文献频道 > 临床内科学 > 文献详细

    文献频道
    • 临床内科
      内科学其他学科
      感染性疾病学
      风湿免疫病学
      分泌代谢病学
      心血管病学
      变态反应学
      神经内科
      肾脏病学
      血液病学
      消化病学
      结核病学
      呼吸病学
    • 临床外科
      泌尿生殖系外科学
      器官移植外科学
      心血管外科学
      外科学其他
      整形外科学
      烧伤外科学
      颅脑外科学
      神经外科学
      显微外科学
      普通外科学
      骨外科学
      胸外科学
    • 临床其他
      精神病与精神卫生学
      影像医学与核医学
      临床检验诊断学
      皮肤病与性病学
      耳鼻咽喉科学
      急诊医学
      老年医学
      口腔医学
      妇产科学
      麻醉学
      眼科学
      护理学
      肿瘤学
      儿科学
      其他
    • 基础医学
      人体解剖学和组织胚胎学
      病理学与病理生理学
      基础医学其他学科
      微生物学与免疫学
      医学寄生虫学
      医学心理学
    • 公共卫生与预防医学
      流行病与卫生统计学
      军事预防医学
      健康教育学
      卫生管理学
      妇幼保健学
      其他
    • 中医中药学
      中西医结合
      针灸推拿学
      民族医学
      中医临床
      中医基础
      中药学
      中医学
    • 药学
      药学其他
      临床药学
      生药学
      药理学
      药剂学
    《皮肤病与性病学》

    叶酸的光降解和皮肤颜色的关系

    发表时间:2010-05-26  浏览次数:549次

      作者:吕小云 张同喜 韩建国 谈笑玲 作者单位:青海大学医学院

      【摘要】 目的 了解叶酸的光降解和皮肤颜色的关系。方法 用荧光光谱仪记录和分析叶酸和维生素B2的光降解过程,用Sigmaplot软件描绘紫外线在不同地区对不同肤色的皮肤的穿透程度。结果 维生素B2的加入可使叶酸在UVA和蓝色光下发生光降解。紫外线穿透肤色类型2最深,类型4最浅.穿透程度随地方的不同而变化。结论 叶酸在紫外线和可见光照射发生降解的事实进一步给“皮肤颜色理论”的可靠性提供了依据。 Lü Xiaoyun(1970~),Male,Tu,Lecturer,Master

      【关键词】 叶酸 黑色素 光降解 皮肤类型

      1。Introduction

      The skin colour is determined by the amount of melanin in the skin. People use skin types 1-4 to represent different skin colours. Type 1 is white, type 2 is less white, type 3 is brown and type 4 is black. Melanin is synthesized from tyrosine in melanocytes and localized in melanosomes. In lightly pigmented skin that has not been exposed to UVB, the melanosomes are found mostly in the basal layer[1]. Melanosomes have relatively high refractive indices (1.55-1.65) compared to the surrounding skin tissue (1.35-1.4) and are therefore important epidermal scatterers. Light with a long wavelength is more strongly scattered from it. Reflectance spectra of skin in the UV spectral region reveal that strongly pigmented skin reflects and scatters more UVB light than the lightly pigmented skin [2]. In response to exposure to UV radiation, melanocytes in the skin can synthesize the dark-brown pigment melanin to prevent UV-induced photolysis of folate and other nutrients [3,4]. Melanin absorbs UV radiation, reduces formation of harmful chemicals called free radicals that form in skin under exposure to UV radiation[5]. The correlation between skin color and latitude is believed to be related to the balancing needs of folate protection and vitamin D production [6].

      A synthetic form of folate, folic acid (FA), is sensitive to UV radiation [7,8]. The most common folate derivative in human blood, 5-methyltetrahydrofolate (5MTHF), is very sensitive to UVB radiation [8]. But UVB penetrates the skin poorly and is not efficient in degrading folate in blood in vivo. UVA cannot degrade folate at all. This fact is unfavorable to skin color theory. However, our investigation reveals that when other vitamin riboflavin is presented, folate can be degraded quickly. There are a lot of vitamins in human skin; the result thus favored the skin color theory again.

      Ultraviolet radiation is traditionally divided into three different regions: UVC (100 - 280), UVB (280 - 320) and UVA (320 - 400). The sun emits electromagnetic radiation from X-rays to radio waves. Due to the ozone layer, dangerous radiation shorter than 290 nm does not reach the surface of the earth. UVB, UVA, visible wavelengths and infrared, are of greatest biological significance. Figure 1 shows the estimated spectral irradiance at noon, midsummer with clear sky and normal ozone: in Oslo, Equator and Lhasa at the Tibetan Plateau. Because of the low latitude, high altitude and low total ozone amount, the Tibetan Plateau is the place with highest UVR on earth [9]. The spectra are calculated by Arne Dahlback, the model used has been compared with measurements and the deviation is within 5 per cent [10,11].

      Fig. 1. Spectral irradiance in Oslo (-), Equator (- -) and Lhasa (……). These spectra are calculated by

      Arne Dahlback, Department of Physics, University of Oslo.

      Materials and Method

      Chemicals: 5-methyltetrahydrofolate (5MTHF) calcium salt from Schircks Laboratories (Jona, Switzerland); Riboflavin from Sigma-Aldrich Chemie (Germany); Dulbecco's phosphate buffered saline (PBS) from PAA laboratories (Austria);

      5-methyltetrahydrofolate (5MTHF) was dissolved in PBS to a concentration of 50 μM, snap frozen in liquid nitrogen and stored in 1 ml tubes at -80℃. For each experiment, 1 ml of the solution (one tube) was diluted in PBS (pH 7.4) to the needed concentration. Because of the instability of 5MTHF, the solutions were always kept on ice before use. Riboflavin were also dissolved in PBS to a concentration of 50 μM and wrapped with aluminium foil and stored in refrigerator. They were diluted into the needed concentration in PBS in each experiment. The temperature of the samples was approximately 25℃. All the experiments were done in dim light to avoid external light exposure.

      Instruments: A Perkin-Elmer UV/VIS spectrophotometer (Lambda 40) and a Perkin-Elmer luminescence spectrometer (LS45); Blue light and UVA radiation source; Quartz suprasil cuvettes, 1.0 × 0.4 cm, 1 mL.

      Software: SigmaPlot 10.0.

      Results and discussion

      Blue light and UVA can not degrade 5MTHF, see figure 2, the absorption spectra remain the same when exposure to blue light and UVA. Riboflavin, however, can be degraded by blue light and UVA. There is an obvious decay at 445 nm.

      Fig. 2. Absorption spectra of 5MTHF and RF alone by blue light exposure. pH 7.4.

      Figure 3 showed the absorption spectra of the mixed solution of 5MTHF and Riboflavin. After subtracting the spectra of riboflavin, we can see that there is an obvious increase at 250nm. As the characteristic spectra of the product of photodegradation of 5MTHF, 5-methyldihydrofolate (5MDHF), the maximum at 250 nm indicate that although 5MTHF is not easily degraded by blue light and UVA, but in the presence of riboflavin, it is degraded and oxidized to 5MDHF quickly.

      Fig. 3. Absorption spectra of 5MTHF + RF by blue light exposure. The absorption spectra of

      5MTHFobtained by subtracting corresponding RF spectra are shown in the right. pH 7.4.

      We have plotted the penetration fluence of different layer of different skin types in figure 4 (a, b, c) according the calculation data from Kristian P.Nielsen et al. [1] It is seen from the graph that light penetrates the lighter pigmented skin deeper than the stronger pigmented skin. Take the different solar spectrum of different places (Equator, Oslo and Lhasa) into account, see figure 2, multiply the solar spectrum of these places with the fluence through epidermis (0.05 mm) (red in the figure), we get part d in figure 4.

      Fig. 4. Different light fluence within different skin type (figure a, b, c). Figure d (1: Oslo;

      2: Equator; 3: Lhasa. Skin type 2 (-); Skin type 3 (-); Skin type 4 (-)

      It was seen from figure 4 that light can reach around 0.3 mm deep in the skin. The deeper in the skin, the less of light reaches. UVA (320 - 400) penetrates more than UVB (280 - 320); UVC (100 - 280) can hardly penetrate the skin. And the deeper the skin colour, the less of light penetrates in the skin. The result also indicates that the altitude and latitude of place have influence to the penetration of light in the skin. High altitude place has the most fluence while the lower latitude place has the lest fluence of penetration in the skin.

      UVC generally does not penetrate the earth's atmosphere. UVB can degrade folate but only arrives to epidermis. Now we have shown that folate can not only be degraded by UVA irradiation which penetrates skin more deeply, but also by visible light that penetrates skin deeper than UVA in the presence of other vitamins like riboflavin. This may be a reason why people living under high solar irradiation need to develop something like melanin to protect this important vitamin. Our investigation thus continued to favour the human skin evolution theory suggested by Branda and Eaton [3], and developed further by Jablonski and Chaplin [6]

      【参考文献】

      [1]Nielsen, K. P., L. Zhao, et al. The importance of the depth distribution of melanin in skin for DNA protection and other photobiological processes[J]. Photochem.Photobiol,2006, 82: 194-198

      [2]Nielsen, K. P., Z. Lu, et al. Reflectance spectra of pigmented and nonpigmented skin in the UV spectral region[J]. Photochem. Photobiol,2004, 80: 450-455

      [3]Branda, R. F. and J. W. Eaton Skin color and nutrient photolysis: an evolutionary hypothesis. Science ,1978,201:625-626

      [4]Cohn, B. A. Sunlight, skin color, and folic acid. [J]. Am. Acad. Dermatol,1978, 46: 317-318

      [5]Jablonski, N. G. and G. Chaplin. Skin deep. Sci, Am.,2002,287: 74-81

      [6]Jablonski, N. G. and G. Chaplin. The evolution of human skin coloration [J]. Hum. Evol,2000, 39:57-106

      [7]Off, M. K., A. E. Steindal, et al. Ultraviolet photodegradation of folic acid[J]. Photochem. Photobiol. 2005, 80: 47-55

      [8]Steindal, A. H., A. Juzeniene, et al. Photodegradation of 5-methyltetrahydrofolate[J]. Photochem. Photobiol, 2006

      [9]Ren, P. B. C., Y. Gjessing, et al. Measurements of solar ultra violet radiation in the Tibetan Plateau and comparisons with discrete ordinate method simulations [J]. Atmos. Sol. Terr. Phys,1999, 61:425-446

      [10]Stamnes, K., S. Chee Tsay, W. Wiscombe, et al. Numerically stable algorithm for discrete-ordinate-method radiative transfer in multiple scattering and emitting layered media[J]. Appl. Optics ,1988,27:2502-2509

      [11]ahlback, A. and K. Stamnes A new spherical model for computing the radiation field available for photolysis and heating rate at twilight[J]. Planet. Space Sci,1991,39:671-683

    ↑上一篇:皮肤热疼痛感与伤害性刺激的关联性
    ↓下一篇:银屑病病人外周血单核细胞TLR2基因表达及血清ASO和IL8水平变化
    全国咨询热线:400-8338-918
    地址:广州市天河区天河北路179号23层2322M房
      粤ICP备2024298770号