The DOI matches its Crossref record; 42 of the 42 references it cites were found in a registry or an index.
A PRECISE WATER ABUNDANCE MEASUREMENT FOR THE HOT JUPITER WASP-43b
Open accessAbstract
The water abundance in a planetary atmosphere provides a key constraint on the planet's primordial origins because water ice is expected to play an important role in the core accretion model of planet formation. However, the water content of the solar system giant planets is not well known because water is sequestered in clouds deep in their atmospheres. By contrast, short-period exoplanets have such high temperatures that their atmospheres have water in the gas phase, making it possible to measure the water abundance for these objects. We present a precise determination of the water abundance in the atmosphere of the 2 M Jup short-period exoplanet WASP-43b based on thermal emission and transmission spectroscopy measurements obtained with the Hubble Space Telescope . We find the water content is consistent with the value expected in a solar composition gas at planetary temperatures (0.4–3.5 × solar at 1σ confidence). The metallicity of WASP-43b's atmosphere suggested by this result extends the trend observed in the solar system of lower metal enrichment for higher planet masses.
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Cites
The Chemical Composition of the Sun
Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145222 · Cited by 9,346
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,127
Analytic Light Curves for Planetary Transit Searches
Mandel, K., & Agol, E. (2002) · The Astrophysical Journal · doi:10.1086/345520 · Cited by 2,256
THE EFFECTS OF SNOWLINES ON C/O IN PLANETARY ATMOSPHERES
Öberg, K. I., Murray-Clay, R., & Bergin, E. A. (2011) · The Astrophysical Journal · doi:10.1088/2041-8205/743/1/l16 · Cited by 1,027
Clouds in the atmosphere of the super-Earth exoplanet GJ 1214b
Kreidberg, L., Bean, J. L., Désert, J.-M., Benneke, B., Deming, D., Stevenson, K. B., Seager, S., Berta-Thompson, Z., Seifahrt, A., & Homeier, D. (2014) · Nature · doi:10.1038/nature12888 · Cited by 939
Self-citationDeming, D., Wilkins, A., McCullough, P., Burrows, A., Fortney, J. J., Agol, E., Dobbs-Dixon, I., Madhusudhan, N., Crouzet, N., Desert, J.-M., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/774/2/95 · Cited by 524
Self-citationMoses, J. I., Visscher, C., Fortney, J. J., Showman, A. P., Lewis, N. K., Griffith, C. A., Klippenstein, S. J., Shabram, M., Friedson, A. J., Marley, M. S., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/737/1/15 · Cited by 490
Self-citationC/O RATIO AS A DIMENSION FOR CHARACTERIZING EXOPLANETARY ATMOSPHERES
Madhusudhan, N. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/758/1/36 · Cited by 465
Self-citationDetection of Carbon Monoxide and Water Absorption Lines in an Exoplanet Atmosphere
Konopacky, Q. M., Barman, T. S., Macintosh, B. A., & Marois, C. (2013) · Science · doi:10.1126/science.1232003 · Cited by 399
Birkby, J. L., de Kok, R. J., Brogi, M., de Mooij, E. J. W., Schwarz, H., Albrecht, S., & Snellen, I. A. G. (2013) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slt107 · Cited by 380
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A chemical survey of exoplanets with ARIEL
Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Heske, A., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G., Puig, L., et al. (2018) · Experimental Astronomy · doi:10.1007/s10686-018-9598-x · Cited by 445
PandExo: A Community Tool for Transiting Exoplanet Science with JWST&HST
Batalha, N. E., Mandell, A., Pontoppidan, K., Stevenson, K. B., Lewis, N. K., Kalirai, J., Earl, N., Greene, T., Albert, L., & Nielsen, L. D. (2017) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/aa65b0 · Cited by 328
Self-citationDomagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136
“This method has also been used to investigate the bulk composition and to detect the presence of clouds in the atmosphere of super-Earth GJ 1416 b (2.7 REarth, 6.5 MEarth; Berta et al., 2012; Kreidberg et al., 2014a).”
Influential
Metadata
- Authors
- Kreidberg, L., Bean, J. L., Désert, J.-M., Line, M. R., Fortney, J. J., Madhusudhan, N., Stevenson, K. B., Showman, A. P., Charbonneau, D., McCullough, P. R., Seager, S., Burrows, A., Henry, G. W., Williamson, M., Kataria, T., & Homeier, D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2014-09-12
- Volume
- 793
- Issue
- 2
- Pages
- L27
- ISSN
- 2041-8205 (ISSN-L)
- 2041-8213
- OpenAlex
- W2100326205
- Cited by
- 401
- References
- 42
- FWCI
- 19.83
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Kreidberg, L., Bean, J. L., Désert, J.-M., Line, M. R., Fortney, J. J., Madhusudhan, N., Stevenson, K. B., Showman, A. P., Charbonneau, D., McCullough, P. R., Seager, S., Burrows, A., Henry, G. W., Williamson, M., Kataria, T., & Homeier, D. (2014). A PRECISE WATER ABUNDANCE MEASUREMENT FOR THE HOT JUPITER WASP-43b. The Astrophysical Journal. https://doi.org/10.1088/2041-8205/793/2/l27
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