E-viri
Recenzirano
Odprti dostop
-
Cortesão, Marta; de Haas, Aram; Unterbusch, Rebecca; Fujimori, Akira; Schütze, Tabea; Meyer, Vera; Moeller, Ralf
Frontiers in microbiology, 04/2020, Letnik: 11Journal Article
The filamentous fungus is one of the main contaminants of the International Space Station (ISS). It forms highly pigmented, airborne spores that have thick cell walls and low metabolic activity, enabling them to withstand harsh conditions and colonize spacecraft surfaces. Whether r spores are resistant to space radiation, and to what extent, is not yet known. In this study, spore suspensions of a wild-type and three mutant strains (with defects in pigmentation, DNA repair, and polar growth control) were exposed to X-rays, cosmic radiation (helium- and iron-ions) and UV-C (254 nm). To assess the level of resistance and survival limits of fungal spores in a long-term interplanetary mission scenario, we tested radiation doses up to 1000 Gy and 4000 J/m . For comparison, a 360-day round-trip to Mars yields a dose of 0.66 ± 0.12 Gy. Overall, wild-type spores of were able to withstand high doses of X-ray (LD = 360 Gy) and cosmic radiation (helium-ion LD = 500 Gy; and iron-ion LD = 100 Gy). Drying the spores before irradiation made them more susceptible toward X-ray radiation. Notably, spores are highly resistant to UV-C radiation (LD = 1038 J/m ), which is significantly higher than that of other radiation-resistant microorganisms (e.g., ). In all strains, UV-C treated spores (1000 J/m ) were shown to have decreased biofilm formation (81% reduction in wild-type spores). This study suggests that spores might not be easily inactivated by exposure to space radiation alone and that current planetary protection guidelines should be revisited, considering the high resistance of fungal spores.
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.