2002
DOI: 10.1016/s0032-0633(02)00010-7
|View full text |Cite
|
Sign up to set email alerts
|

Exposure of amino acids and derivatives in the Earth orbit

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
11
0

Year Published

2004
2004
2011
2011

Publication Types

Select...
3
3

Relationship

0
6

Authors

Journals

citations
Cited by 24 publications
(12 citation statements)
references
References 21 publications
1
11
0
Order By: Relevance
“…This amino acid is also used in the photosystem II of chloroplasts, acting as the electron donor of the oxidized chlorophyll. Tyrosine, because of its aromatic ring, absorbs strongly at 280 nm (Chang, 2000) and, like RNA/DNA in water, has demonstrated chemical stability under high doses of UV radiation (Barbiera et al, 2002), suggesting that its initial association with RNA/DNA may have been as a robust antenna type of photon absorber to augment the local water temperature sufficiently for denaturation.…”
Section: Evolutionmentioning
confidence: 99%
“…This amino acid is also used in the photosystem II of chloroplasts, acting as the electron donor of the oxidized chlorophyll. Tyrosine, because of its aromatic ring, absorbs strongly at 280 nm (Chang, 2000) and, like RNA/DNA in water, has demonstrated chemical stability under high doses of UV radiation (Barbiera et al, 2002), suggesting that its initial association with RNA/DNA may have been as a robust antenna type of photon absorber to augment the local water temperature sufficiently for denaturation.…”
Section: Evolutionmentioning
confidence: 99%
“…Irradiation experiments were performed at room temperature (290 K) because the temperature of exposed cells in low Earth orbit was about 230-310 K (Barbier et al 1998;Barbier et al 2002;Boillot et al 2002;Guan et al 2010). Each film was irradiated with VUV light with an energy of 7.2 eV (FWHM~0.5 eV, wavelength l=172 nm) using a Xe 2 * excimer lamp (UER20H-172A, USHIO) under vacuum (pressure<10 −4 Pa) for 20, 30, 60, 240 or 600 s. The irradiation flux p was determined to be 5.4×10 15 photons cm −2 s −1 using a calibrated photodiode (S1337-1010BQ, Hamamatsu Photonics).…”
Section: Vuv Irradiationmentioning
confidence: 99%
“…The photo-stability of pure amino acids under polychromatic ultraviolet irradiation has been examined at low Earth orbit (Barbier et al 1998;Barbier et al 2002;Boillot et al 2002;Cottin et al 2008;Guan et al 2010) and in laboratories (Ehrenfreund et al 2001;ten Kate et al 2005). However, as Schwell et al (2006) have already stated, it is also important to examine the decomposition and oligomerization rates induced by monochromatic light to understand the photochemistry of extraterrestrial organic molecules.…”
Section: Introductionmentioning
confidence: 99%
“…We have already shown that amino acid synthesis is possible inside cometary grains under interstellar environment conditions (Munoz Caro, 2002). We are now interested in the effects of space conditions and meteoritic impact on these amino acids (Cottin, 2008;Barbier, 2002;Boillot, 2002). Most of the extraterrestrial organic molecules known today have been identified in carbonaceous chondrite meteorites (Cronin, 1993).…”
Section: Formation Of Protonated Methanimine As a Keymentioning
confidence: 99%