Abstract
Spectra of Triton with a CCD spectrometer yielded a relative spectral reflectivity curve from 0.56 to 1.05 μm at a resolution of 25 Å. Using low-temperature band model parameters from Fink et al. (1980), an upper limit for the one-way path gaseous CH4 abundance of 1 m-am was derived.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 288-291 |
| Number of pages | 4 |
| Journal | Icarus |
| Volume | 46 |
| Issue number | 2 |
| DOIs | |
| State | Published - 1981 |
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ASJC Scopus subject areas
- Space and Planetary Science
- Astronomy and Astrophysics
Cite this
Spectrophotometry and upper limit of gaseous CH4 for Triton. / Johnson, James R.; Fink, Uwe -; Smith, Bradford A.; Reitsema, H. J.
In: Icarus, Vol. 46, No. 2, 1981, p. 288-291.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Spectrophotometry and upper limit of gaseous CH4 for Triton
AU - Johnson, James R.
AU - Fink, Uwe -
AU - Smith, Bradford A.
AU - Reitsema, H. J.
PY - 1981
Y1 - 1981
N2 - Spectra of Triton with a CCD spectrometer yielded a relative spectral reflectivity curve from 0.56 to 1.05 μm at a resolution of 25 Å. Using low-temperature band model parameters from Fink et al. (1980), an upper limit for the one-way path gaseous CH4 abundance of 1 m-am was derived.
AB - Spectra of Triton with a CCD spectrometer yielded a relative spectral reflectivity curve from 0.56 to 1.05 μm at a resolution of 25 Å. Using low-temperature band model parameters from Fink et al. (1980), an upper limit for the one-way path gaseous CH4 abundance of 1 m-am was derived.
UR - http://www.scopus.com/inward/record.url?scp=49049148113&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=49049148113&partnerID=8YFLogxK
U2 - 10.1016/0019-1035(81)90218-9
DO - 10.1016/0019-1035(81)90218-9
M3 - Article
AN - SCOPUS:49049148113
VL - 46
SP - 288
EP - 291
JO - Icarus
JF - Icarus
SN - 0019-1035
IS - 2
ER -