Transmission spectroscopy enables the detection of atmospheres on extrasolar planets.
Is it true that transmission spectroscopy enables the detection of atmospheres on extrasolar planets?
Yes. Transmission spectroscopy is a foundational and proven observational technique that enables the detection and characterization of extrasolar planet atmospheres.
Verdict: SUPPORTED · 7 sources for, 0 against · Last checked
The retrieved papers consistently demonstrate that transmission spectroscopy is widely used and mathematically modeled to detect, retrieve, and analyze the atmospheric compositions of transiting exoplanets, supported by major space missions such as Hubble, TESS, ARIEL, and JWST.
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Ricker, G., Winn, J. N., Vanderspek, R., Latham, D. W., Bakos, G. Á., Bean, J. L., Berta-Thompson, Z. K., Brown, T. M., Buchhave, L. A., Butler, N., Butler, R. P., Chaplin, W. J., Charbonneau, D., Christensen‐Dalsgaard, J., Clampin, M., Deming, D., Doty, J., Lee, N. D., Dressing, C. D., Dunham, E. W., Endl, M., Fressin, F., Ge, J., Henning, T., Holman, M. J., Howard, A. W., Ida, S., Jenkins, J. M., Jernigan, G., Johnson, J. A., Kaltenegger, L., Kawai, N., Kjeldsen, H., Laughlin, G., Levine, A. M., Lin, D. N. C., Lissauer, J. J., MacQueen, P. J., Marcy, G. W., McCullough, P. R., Morton, T. D., Narita, N., Paegert, M., Πάλλη, Ε., Pepe, F., Pepper, J., Quirrenbach, A., Rinehart, S. A., Sasselov, D., Sato, B., Seager, S., Sozzetti, A., Stassun, K. G., Sullivan, P., Szentgyorgyi, A., Torres, G., Udry, S., & Villaseñor, J. (2014). Transiting Exoplanet Survey Satellite. doi.org. https://doi.org/10.1117/1.jatis.1.1.014003
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Kempton, E. M., Bean, J. L., Louie, D. R., Deming, D., Koll, D. D. B., Mansfield, M., Christiansen, J. L., López‐Morales, M., Swain, M. R., Zellem, R. T., Ballard, S., Barclay, T., Barstow, J. K., Batalha, N. E., Beatty, T. G., Berta-Thompson, Z. K., Birkby, J., Buchhave, L. A., Charbonneau, D., Cowan, N. B., Crossfield, I. J. M., Val-Borro, M. d., Doyon, R., Dragomir, D., Gaidos, E., Heng, K., Hu, R., Kane, S. R., Kreidberg, L., Mallonn, M., Morley, C., Narita, N., Nascimbeni, V., Πάλλη, Ε., Quintana, E. V., Rauscher, E., Seager, S., Shkolnik, E. L., Sing, D. K., Sozzetti, A., Stassun, K. G., Valenti, J. A., & Essen, C. v. (2018). A Framework for Prioritizing the <i>TESS</i> Planetary Candidates Most Amenable to Atmospheric Characterization. doi.org. https://doi.org/10.1088/1538-3873/aadf6f
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Pont, F., Knutson, H. A., Gilliland, R. L., Moutou, C., & Charbonneau, D. (2008). Detection of atmospheric haze on an extrasolar planet: the 0.55-1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope. doi.org. https://doi.org/10.1111/j.1365-2966.2008.12852.x
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Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Heske, A., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G. L., Puig, L., Turrini, D., Vandenbussche, B., Wolkenberg, P., Beaulieu, J., Buchave, L. A., Ferus, M., Griffin, M., Guêdel, M., Justtanont, K., Lagage, P., Machado, P., Malaguti, G., Min, M., Nørgaard-Nielsen, H. U., Rataj, M., Ray, T., Ribas, I., Swain, M. G., Szabó, R., Werner, S., Barstow, J. K., Burleigh, M. R., Cho, J., Foresto, V. C. d., Coustenis, A., Decin, L., Encrenaz, T., Galand, M., Gillon, M., Helled, R., Morales, J. C., Muñoz, A. G., Moneti, A., Pagano, I., Pascale, E., Piccioni, G., Pinfield, D. J., Sarkar, S., Selsis, F., Tennyson, J., Triaud, A. H. M. J., Vénot, O., Waldmann, I., Waltham, D., Wright, G., Amiaux, J., Auguères, J., Berthé, M., Bezawada, N., Bishop, G., Bowles, N. E., Coffey, D., Colomé, J., Crook, M., Crouzet, P., Peppo, V. D., Sanz, I. E., Focardi, M., Frericks, M., Hunt, T., Kohley, R., Middleton, K., Morgante, G., Ottensamer, R., Pace, E., Pearson, C., Stamper, R., Symonds, K., Rengel, M., Renotte, É., Ade, P. A. R., Affer, L., Alard, C., Allard, N. F., Altieri, F., André, Y., Arena, C., Argyriou, I., Aylward, A. D., Baccani, C., Bakos, G. Á., Banaszkiewicz, M., Barlow, M., Batista, V., Bellucci, G., Benatti, S., Bernardi, P., Bézard, B., Błęcka, M. I., & Bolmont, É. (2018). A chemical survey of exoplanets with ARIEL. doi.org. https://doi.org/10.1007/s10686-018-9598-x
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Benneke, B. & Seager, S. (2012). ATMOSPHERIC RETRIEVAL FOR SUPER-EARTHS: UNIQUELY CONSTRAINING THE ATMOSPHERIC COMPOSITION WITH TRANSMISSION SPECTROSCOPY. doi.org. https://doi.org/10.1088/0004-637x/753/2/100
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Lustig-Yaeger, J., Meadows, V. S., & Lincowski, A. P. (2019). The Detectability and Characterization of the TRAPPIST-1 Exoplanet Atmospheres with JWST. doi.org. https://doi.org/10.3847/1538-3881/ab21e0
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Team, J. T. E. C. E. R. S., Ahrer, E., Alderson, L., Batalha, N. M., Batalha, N., Batalha, N. E., Batalha, N. E., Bean, J. L., Beatty, T. G., Bell, T. J., Benneke, B., Berta-Thompson, Z. K., Carter, A. L., Crossfield, I. J. M., Espinoza, N., Feinstein, A. D., Fortney, J. J., Gibson, N. P., Goyal, J., Kempton, E. M., Kirk, J., Kreidberg, L., López-Morales, M., Line, M. R., Lothringer, J. D., Moran, S. E., Mukherjee, S., Ohno, K., Parmentier, V., Piaulet, C., Rustamkulov, Z., Schlawin, E., Sing, D. K., Stevenson, K. B., Wakeford, H. R., Allen, N. H., Birkmann, S. M., Brande, J., Crouzet, N., Cubillos, P. E., Damiano, M., Désert, J., Peter, G., Harrington, J., Hu, R., Kendrew, S., Knutson, H. A., Lagage, P., Leconte, J., Lendl, M., MacDonald, R. J., May, E. M., Miguel, Y., Molaverdikhani, K., Moses, J. I., Murray, C. A., Nehring, M., Nikolov, N. K., Roche, D. J. M. P. d. d. l., Radica, M., Roy, P., Stassun, K. G., Taylor, J., Waalkes, W. C., Wachiraphan, P., Welbanks, L., Wheatley, P., Aggarwal, K., Alam, M. K., Banerjee, A., Barstow, J. K., Blecic, J., Casewell, S. L., Changeat, Q., Chubb, K. L., Colón, K. D., Coulombe, L., Daylan, T., Val-Borro, M. d., Decin, L., Santos, L. A. D., Flagg, L., France, K., Fu, G., Muñoz, A. G., Gizis, J. E., Glidden, A., Grant, D., Hong, Y., Henning, T., Hong, Y., Inglis, J., Iro, N., Kataria, T., Komacek, T. D., Krick, J., Lee, E. K. H., Lewis, N. K., Lillo-Box, J., & Lustig‐Yaeger, J. (2022). Identification of carbon dioxide in an exoplanet atmosphere. doi.org. https://doi.org/10.1038/s41586-022-05269-w
What does the evidence say?
The retrieved papers consistently demonstrate that transmission spectroscopy is widely used and mathematically modeled to detect, retrieve, and analyze the atmospheric compositions of transiting exoplanets, supported by major space missions such as Hubble, TESS, ARIEL, and JWST.
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