Academic literature on the topic 'Exoplanets'
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Journal articles on the topic "Exoplanets"
Montemor, Ryan Nepomuceno, and Ricardo Roberto Plaza Teixceira. "Atividades de divulgação científica sobre exoplanetas." Revista Brasileira de Educação em Ciências e Educação Matemática 5, no. 2 (August 31, 2021): 445–60. http://dx.doi.org/10.33238/rebecem.2021.v.5.n.2.26865.
Full textVarela, J., V. Réville, A. S. Brun, P. Zarka, and F. Pantellini. "Effect of the exoplanet magnetic field topology on its magnetospheric radio emission." Astronomy & Astrophysics 616 (August 2018): A182. http://dx.doi.org/10.1051/0004-6361/201732091.
Full textLi, Megan G., Sofia Z. Sheikh, Christian Gilbertson, Matthias Y. He, Howard Isaacson, Steve Croft, and Evan L. Sneed. "Developing a Drift Rate Distribution for Technosignature Searches of Exoplanets." Astronomical Journal 166, no. 5 (October 17, 2023): 182. http://dx.doi.org/10.3847/1538-3881/acf83d.
Full textWang, Zhixin. "Extrasolar Planet Candidates Identified by Single Transit from TESS." Journal of Physics: Conference Series 2441, no. 1 (March 1, 2023): 012030. http://dx.doi.org/10.1088/1742-6596/2441/1/012030.
Full textUlmer-Moll, S., N. C. Santos, P. Figueira, J. Brinchmann, and J. P. Faria. "Beyond the exoplanet mass-radius relation." Astronomy & Astrophysics 630 (October 2019): A135. http://dx.doi.org/10.1051/0004-6361/201936049.
Full textYang, Gilbert. "Detection of Exoplanets based on the Transit Method." Highlights in Science, Engineering and Technology 31 (February 10, 2023): 196–203. http://dx.doi.org/10.54097/hset.v31i.5140.
Full textGupta, Richa, and Sidratul Muntaha. "Identifying Potentially Habitable Exoplanets: A Study using the Transit Method and Kepler dataset." Applied and Computational Engineering 8, no. 1 (August 1, 2023): 93–97. http://dx.doi.org/10.54254/2755-2721/8/20230089.
Full textAshtari, Reza, Anthony Sciola, Jake D. Turner, and Kevin Stevenson. "Detecting Magnetospheric Radio Emission from Giant Exoplanets." Astrophysical Journal 939, no. 1 (October 28, 2022): 24. http://dx.doi.org/10.3847/1538-4357/ac92f5.
Full textSokoloff, Dmitry, Helmi Malova, and Egor Yushkov. "Symmetries of Magnetic Fields Driven by Spherical Dynamos of Exoplanets and Their Host Stars." Symmetry 12, no. 12 (December 15, 2020): 2085. http://dx.doi.org/10.3390/sym12122085.
Full textLigi, Roxanne, Denis Mourard, Karine Perraut, Philippe Bério, Lionel Bigot, Andrea Chiavassa, Anne-Marie Lagrange, and Nicolas Nardetto. "Modeling transiting exoplanet and spots For interferometric study." Proceedings of the International Astronomical Union 9, S302 (August 2013): 202–5. http://dx.doi.org/10.1017/s1743921314002087.
Full textDissertations / Theses on the topic "Exoplanets"
Baroch, López David. "Analysis of high-precision spectroscopic and photometric data for planet and stellar characterisation." Doctoral thesis, Universitat Autònoma de Barcelona, 2021. http://hdl.handle.net/10803/673657.
Full textLa detección de la primera estrella binaria hace más de 200 años representó el inicio de un nuevo campo en la astrofísica dedicado al estudio de la evolución y las interacciones de estos sistemas, usando como principal herramienta el análisis del movimiento reflejo causado por el cuerpo orbitante. Solo fue cuestión de tiempo que los instrumentos de medida alcanzaran un nivel de precisión suficientemente elevado como para detectar los movimientos inducidos por planetas sobre sus estrellas. El descubrimiento del primer exoplaneta hace casi tres décadas supuso la creación de un seguido de proyectos dedicados a la búsqueda de nuevos mundos, los cuales están produciendo un montón de datos que se están usando con la finalidad de estudiar diferentes propiedades de las estrellas. El objetivo principal de esta tesis es el estudio y caracterización de exoplanetas, estrellas y sistemas estelares mediante el análisis de datos provenientes de proyectos dedicados a la busca de exoplanetas con instrumentos de alta precisión. Este es el caso de los proyectos CARMENES y TESS, que tienen el objetivo de encontrar planetas usando el método de la velocidad radial y la detección de tráficos planetarios, respectivamente, poniendo un énfasis especial en estrellas tipo M. Primeramente, hemos desarrollado un nuevo método para determinar las propiedades de las manchas estelares y de los movimientos convectivos en estrellas M usando la variabilidad inducida por la actividad estelar. En particular, hemos modelado las velocidades radiales cromáticas y la fotometría de la estrella YZ CMi usando el software de modelado de actividad estelar StarSim. El análisis ha revelado la presencia de una gran mancha polar con una temperatura 200 K inferior a la de la estrella, encontrando también que el movimiento convectivo de la estrella podría tener un movimiento inverso al esperado. A partir de un análisis combinado de velocidades radiales antiguas y de CARMENES, en esta tesis presentamos la detección de un mini Neptuno y una supertierra alrededor de las estrellas M LSPM J2116+0234 y GJ 686, respectivamente, justo fuera del límite interno de las respectivas zonas habitables. Para evitar la determinación sesgada de las características de los planetas, hemos modelado las señales planetarias conjuntamente con las provenientes de la actividad estelar, los cuales hemos modelado con ruido correlacionado. Los parámetros orbitales resultantes de este análisis corresponden a periodos orbitales de 14.45 d y 15.53 d, y masas mínimas de 12.8 y 6.6 masas terrestres para los planetas LSPM J2116+0234b y GJ 686b, respectivamente. El método de velocidades radiales empleado para detectar exoplanetas con CARMENES también permite la detección de sistemas múltiples. En este trabajo, anunciamos el descubrimiento de 17 nuevos sistemas, de los cuales determinamos las órbitas espectrales. La muestra está formada por 15 sistemas binarios (5 con compañeras no detectadas) y 3 sistemas triples. Hemos determinado que las compañeras no detectadas de dos de las binarias tienen masas mínimas compatibles con una enana marrón, y demostramos que un sistema binario está formado por una enana blanca y una estrella M. Un análisis conjunto de velocidades radiales y astrometría nos ha permitido determinar las masas de un sistema binario, el cual es uno de los sistemas más jóvenes con masas medidas. Por último, hemos usado fotometría de TESS para determinar el tiempo de eclipse de 16 binarias eclipsantes excéntricas. Mediante el análisis de la evolución de las diferencias entre el tiempo de eclipse primario y secundario con el tiempo, hemos determinado el movimiento apsidal de 10 sistemas, 5 de los cuales son medidos por primera vez. Hemos comparado nuestras medidas con predicciones teóricas obteniendo una concordancia excelente. Hemos sido capaces de medir el término relativista con suficiente precisión para testar la relatividad general con este método por primera vez.
The detection of the first binary star more than 200 years ago opened the door to a whole new field of astrophysics research, devoted to the study of their evolution and mutual interactions employing the analysis of the reflex motion caused by the orbiting companion. It was therefore only a matter of time that the development of astronomical instrumentation reached a precise enough level to detect the motions induced by planetary companions over their host stars. The discovery of the first exoplanet a few decades ago prompted a rapid surge of surveys dedicated to their search, which are providing a huge amount of data that can be also used to study the properties of stars. The main purpose of this thesis is the study and characterization of exoplanets, stars, and stellar systems by analyzing data from high-precision spectroscopic and photometric exoplanet surveys. This is for instance the case of the CARMENES and TESS projects, which aim at the discovery of such objects by means of the radial velocity imprinted on their host star or by the detection of transits, respectively, with particular emphasis on low-mass M-dwarf stars. Firstly, we developed a novel approach to constraint the properties of starspots and convective motions on M dwarfs by using the variability induced by stellar activity. In particular, we modeled chromatic radial velocities and photometric time series of the M-dwarf star YZ CMi using the stellar activity model code StarSim. The results of our analysis revealed the presence of a large polar spot with a temperature 200 K lower than that of the surrounding photosphere, and found that the convective shift of this star may be reversed toward redshift. Based on a combined analysis of CARMENES and archival radial velocities, we present in this thesis the detection of a mini-Neptune and a super-Earth around the M-dwarf stars LSPM J2116+0234 and GJ 686, respectively, just outside the inner edge of their habitable zones. To avoid determining biased parameters due to the contamination from stellar activity, the planetary signals were jointly modeled with a correlated noise model describing stellar variability. The derived orbital parameters resulted in orbital periods of 14.45 d and 15.53 d, and minimum masses of 12.8 and 6.6 Earth masses for LSPM J2116+0234b and GJ 686b, respectively. The radial velocity method used to detect exoplanets with CARMENES is also yielding multiple stellar systems as a by-product. In this work, we report on the discovery of 17 new multiple systems, for which we determined their spectroscopic orbits. The sample is composed of 15 binary systems (5 with undetected companions) and 2 triple systems. We determined that the unseen companions of two of the binaries have minimum masses compatible with a brown dwarf, and we demonstrated that one of the systems is an M-dwarf--white dwarf binary. We also found one of the youngest binary systems with measured masses by analysing both radial velocities and astrometric measurements. Finally, we used TESS photometry to derive eclipse timings for 16 well-studied eccentric eclipsing binaries. We analyzed the change in the difference between primary and secondary eclipse timings over time to determine the apsidal motion rate of 10 of the systems in the sample, 5 of which are measured for the first time. We compared the measured values with theoretical predictions, obtaining an excellent agreement. We were able to measure the general relativistic.
Universitat Autònoma de Barcelona. Programa de Doctorat en Física
Lafarga, Magro Marina. "Stellar activity and exoplanets ofMdwarfs from CARMENES visible to near-infrared spectroscopy." Doctoral thesis, Universitat Autònoma de Barcelona, 2020. http://hdl.handle.net/10803/671618.
Full textDespués del descubrimiento de los primeros exoplanetas hace unas tres décadas, la detección y caracterización de compañeros planetarios se ha convertido en un tema de investigación prominente, especialmente la búsqueda de planetas parecidos a la Tierra, cuerpos rocosos que orbitan en la zona habitable (HZ) de sus estrellas huéspedes. Uno de los principales métodos utilizados para encontrar y caracterizar exoplanetas es la técnica de la espectroscopía Doppler o velocidad radial (RV), basada en el uso de espectros estelares para medir cambios periódicos en la RV de una estrella causados por la atracción gravitatoria de un exoplaneta en órbita. Actualmente, la variabilidad intrínseca de las estrellas huéspedes es el principal reto en el estudio de exoplanetas. Las estrellas no son cuerpos invariables ni homogéneos, sino que presentan variabilidad en distintas escalas de tiempo. La más relevante es la actividad magnética estelar, que incluye fenómenos como manchas o fáculas que aparecen en la superficie de la estrella y están moduladas por su rotación. Estos fenómenos distorsionan los espectros estelares, introduciendo sesgos en las RVs suficientemente grandes como para esconder o hasta imitar la señal causada por un planeta. Por lo tanto, para continuar detectando y estudiando exoplanetas de baja masa, una mejor comprensión de estos fenómenos estelares y sus efectos en nuestras observaciones es clave. Esta tesis se centra en el estudio de los efectos de la actividad estelar en observaciones espectroscópicas de estrellas frías obtenidas con el instrumento CARMENES. CARMENES es un espectrógrafo de alta resolución capaz de observar en el rango de longitudes de onda visible e infrarojo cercano. Está realizando un estudio de más de 300 enanas M, las estrellas con menor masa de la secuencia principal, con el objetivo primordial de detectar exoplanetas pequeños. En primer lugar, hemos desarrollado un código que implementa el método de la función de correlación cruzada (CCF) para medir RVs e indicadores de actividad estelar en observaciones de alta resolución, y lo hemos aplicado a los datos de CARMENES. Este método usa máscaras binarias ponderadas, un template estelar simplificado construido seleccionando líneas espectrales. Hemos creado varias máscaras en función del subtipo espectral y de la velocidad de rotación de la estrella a analizar. A continuación, hemos utilizado los indicadores de actividad derivados de la CCF, juntamente con otros indicadores de actividad espectroscópicos, para analizar sus variaciones temporales en una muestra de casi 100 enanas M de varias masas y niveles de actividad. Aproximadamente la mitad de las estrellas analizadas muestran RVs con señales de actividad claros. Distintos indicadores son sensibles a la actividad de forma diferente según las características de la estrella: indicadores cromosféricos son más útiles para estrellas de baja actividad, indicadores relacionados con el cambio de RV con la longitud de onda funcionan mejor para estrellas más activas, y otros indicadores relacionados con el cambio de anchura de las líneas fotosféricas proporcionan resultados similares en todo tipo de estrellas, pero son especialmente útiles para las más activas y de menor masa. Finalmente, hemos analizado los efectos de la actividad sobre líneas de absorción individuales presentes en el espectro de estrellas activas. Estudiando las correlaciones entre las RVs de líneas individuales y los indicadores de actividad, podemos clasificar las líneas observadas según su sensibilidad a la actividad. Esto nos permite seleccionar líneas afectadas de forma distinta por la actividad y usarlas para volver a calcular RVs. De esta forma obtenemos RVs para las cuales mitigamos o incrementamos la señal de actividad en diversos grados. También observamos que las mismas líneas en distintas estrellas muestran diferente sensibilidad a la actividad.
After the discovery of the first exoplanets about three decades ago, the detection and characterization of planetary companions has become a prominent research topic, especially the search for Earth-like planets, rocky bodies orbiting in the habitable zone (HZ) of their host stars. One of the main methods used to find and characterise exoplanets is the Doppler spectroscopy or radial velocity (RV) technique, based on using stellar spectra to measure periodic changes in the RV of a star caused by the gravitational pull of an orbiting exoplanet. Currently, the intrinsic variability of the host stars is the major challenge faced in the study of exoplanets. Stars are not quiet, homogeneous bodies, but display variability on different timescales, the most concerning being stellar magnetic activity, phenomena such as spots or faculae appearing on the stellar surface and modulated by the stellar rotation. These features distort the stellar spectra, introducing biases in our RVs that can be large enough to hide or even mimic the signal caused by a planet. Therefore, to continue detecting and studying low-mass exoplanets, a better understanding of these stellar phenomena and their effects on our observations is key. This thesis is focused on the study of stellar activity effects on spectroscopic observations of cool stars obtained with the CARMENES instrument. CARMENES is a high-resolution spectrograph capable of observing on the visible and near-infrared wavelength ranges. It is performing a survey of over 300 M dwarfs, stars at the low-mass end of the main sequence, with the main goal of detecting small exoplanets. Firstly, we developed a pipeline that implements the cross-correlation function (CCF) method to measure RVs and indicators of stellar activity on high-resolution observations, and applied it to the CARMENES survey data. This method uses weighted binary masks, a simplified stellar template built by selecting sharp spectral lines, of which we created different kinds depending on the spectral subtype and the rotational velocity of the target star. We then used the activity indicators derived from the CCF, together with other spectroscopic activity proxies, to analyse their temporal variations in a sample of almost 100 M dwarfs with a range of masses and activity levels. We found that about half of the stars analysed show RVs with clear signals of activity. Different indicators trace activity differently depending on the characteristics of the star: chromospheric indicators are the most useful for low-activity stars, indicators related to the change in RV with wavelength work better for the most active stars, and other indicators related to the change in width of the photospheric lines provide similar results in all types of stars, but are especially useful for the most active and lowest-mass ones. Finally, we analysed the effects of activity on individual absorption features present on the spectra of active stars. By studying the correlations between the individual line RVs and activity indicators, we are able to classify the observed lines according to their sensitivity to activity. This allow us to select differently affected lines and use them to recompute RVs for which we mitigate or enhance the activity signal to varying degrees. We also observe that the same lines on different stars show different sensitivities to activity.
Bochinski, Jakub Jaroslaw. "Observations of transiting exoplanets." Thesis, Open University, 2016. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.699818.
Full textFrith, James Michael. "Towards atmospheric characterisation of exoplanets." Thesis, University of Hertfordshire, 2014. http://hdl.handle.net/2299/14247.
Full textSvensson, Rebecka. "Exploring the Diversity of Exoplanets." Thesis, Luleå tekniska universitet, Institutionen för system- och rymdteknik, 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-87402.
Full textBrothwell, Rayn David. "The dynamic nature of exoplanets." Thesis, Queen's University Belfast, 2016. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.705899.
Full textPearson, Kyle A., Leon Palafox, and Caitlin A. Griffith. "Searching for exoplanets using artificial intelligence." OXFORD UNIV PRESS, 2018. http://hdl.handle.net/10150/627143.
Full textHodosán, Gabriella. "Lightning on exoplanets and brown dwarfs." Thesis, University of St Andrews, 2017. http://hdl.handle.net/10023/12079.
Full textGeorgieva, Iskra. "Searching for Exoplanets in K2 Data." Thesis, Luleå tekniska universitet, Rymdteknik, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-70960.
Full textArmstrong, David John. "On the abundance of circumbinary exoplanets." Thesis, University of Warwick, 2015. http://wrap.warwick.ac.uk/72676/.
Full textBooks on the topic "Exoplanets"
Mason, John W., ed. Exoplanets. Berlin, Heidelberg: Springer Berlin Heidelberg, 2008. http://dx.doi.org/10.1007/978-3-540-74008-7.
Full textKitchin, Chris. Exoplanets. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-0644-0.
Full textSimon, Seymour. Exoplanets. New York, NY: HarperCollins Publishers, 2018.
Find full textExoplanets. San Diego, CA: Sally Ride Science, 2008.
Find full textExploring exoplanets. Minneapolis: Lerner Publications, 2012.
Find full textDeeg, Hans J., and Juan Antonio Belmonte, eds. Handbook of Exoplanets. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-319-30648-3.
Full textBozza, Valerio, Luigi Mancini, and Alessandro Sozzetti, eds. Methods of Detecting Exoplanets. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-27458-4.
Full textFormation and evolution of exoplanets. Weinheim: Wiley-VCH, 2010.
Find full textKitchin, C. R. Exoplanets: Finding, exploring, and understanding alien worlds. New York: Springer, 2012.
Find full textMusielak, Zdzislaw, and Billy Quarles. Three Body Dynamics and Its Applications to Exoplanets. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-58226-9.
Full textBook chapters on the topic "Exoplanets"
Inglis, Michael. "Exoplanets." In The Patrick Moore Practical Astronomy Series, 225–38. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-11644-0_13.
Full textKarttunen, Hannu, Pekka Kröger, Heikki Oja, Markku Poutanen, and Karl Johan Donner. "Exoplanets." In Fundamental Astronomy, 459–62. Berlin, Heidelberg: Springer Berlin Heidelberg, 2016. http://dx.doi.org/10.1007/978-3-662-53045-0_22.
Full textRice, Ken. "Exoplanets." In Handbook of Astrobiology, 759–73. Boca Raton, Florida : CRC Press, [2019]: CRC Press, 2018. http://dx.doi.org/10.1201/b22230-50.
Full textJagadeesh, Madhu Kashyap, and Usha Shekhar. "Exoplanets." In Extreme Habitable Environments, 42–50. New York: CRC Press, 2022. http://dx.doi.org/10.1201/9780429289590-3.
Full textInglis, Michael. "Exoplanets." In The Patrick Moore Practical Astronomy Series, 331–50. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-16805-5_15.
Full textKitchin, Chris. "Because We Live on One! – or – Why Planets and Exoplanets Are Important." In Exoplanets, 1–6. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0644-0_1.
Full textKitchin, Chris. "On the Track of Alien Planets – Other Approaches (0% of All Exoplanet Primary Discoveries)." In Exoplanets, 133–42. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0644-0_10.
Full textKitchin, Chris. "Where Do We Go from Here? – Future Approaches to Exoplanet Detection and Study." In Exoplanets, 143–55. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0644-0_11.
Full textKitchin, Chris. "Exoplanets Revealed – What They Are Really Like." In Exoplanets, 157–90. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0644-0_12.
Full textKitchin, Chris. "Exoplanets and Exoplanetary Systems: Pasts and Futures." In Exoplanets, 191–202. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0644-0_13.
Full textConference papers on the topic "Exoplanets"
Avtaeva, A., and V. Shematovich. "Comparison of non-thermal atmospheric losses for hot exoplanets." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.074.
Full textIpatov, S. I. "Migration of planetesimals to planets located in habitable zones in the Solar System and in the Proxima Centauri system." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.084.
Full textAlbrecht, Simon. "Exoplanets." In Frank N. Bash Symposium 2011: New Horizons in Astronomy. Trieste, Italy: Sissa Medialab, 2012. http://dx.doi.org/10.22323/1.149.0002.
Full textRusso, Matt, and Andrew Santaguida. "5000 Exoplanets: Listen to the Sounds of Discovery." In ICAD 2022: The 27th International Conference on Auditory Display. icad.org: International Community for Auditory Display, 2022. http://dx.doi.org/10.21785/icad2022.023.
Full textDandumont, Colin, Jens Kammerer, Denis Defrère, and Jérôme Loicq. "Performance study of interferometric small-sats to detect exoplanets: updated exoplanet yield and application to nearby exoplanets." In Optical and Infrared Interferometry and Imaging VII, edited by Antoine Mérand, Stephanie Sallum, and Peter G. Tuthill. SPIE, 2020. http://dx.doi.org/10.1117/12.2562119.
Full textSmith, Christopher J., Geronimo L. Villanueva, and Gabrielle Suissa. "Imagining Exoplanets." In SIGGRAPH '20: Special Interest Group on Computer Graphics and Interactive Techniques Conference. New York, NY, USA: ACM, 2020. http://dx.doi.org/10.1145/3388767.3407354.
Full textSmith, Matthew W., Sara Seager, Christopher M. Pong, Jesus S. Villaseñor, George R. Ricker, David W. Miller, Mary E. Knapp, Grant T. Farmer, and Rebecca Jensen-Clem. "ExoplanetSat: detecting transiting exoplanets using a low-cost CubeSat platform." In SPIE Astronomical Telescopes + Instrumentation, edited by Jacobus M. Oschmann, Jr., Mark C. Clampin, and Howard A. MacEwen. SPIE, 2010. http://dx.doi.org/10.1117/12.856559.
Full textClaudi, Riccardo. "Exoplanets: Possible Biosignatures." In Frontier Research in Astrophysics – II. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.269.0061.
Full textSchneider, J. "Exoplanets: Which wavelengths?" In Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg, edited by Torben E. Andersen. SPIE, 2008. http://dx.doi.org/10.1117/12.801262.
Full textRovithis-Livaniou, Eleni, Vasile Mioc, Cristiana Dumitrache, and Nedelia A. Popescu. "Exoplanets: An Overview." In EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993675.
Full textReports on the topic "Exoplanets"
Smullen, Rachel. Exoplanets: Strange New Worlds. Office of Scientific and Technical Information (OSTI), April 2021. http://dx.doi.org/10.2172/1779647.
Full textLunine, J., D. Fischer, H. Hammel, L. Hillenbrand, J. Kasting, G. Laughlin, B. Macintosh, et al. Worlds Beyond: A Strategy for the Detection and Characterization of Exoplanets. Office of Scientific and Technical Information (OSTI), June 2008. http://dx.doi.org/10.2172/945593.
Full textZilberman, Mark. Shouldn’t Doppler 'De-boosting' be accounted for in calculations of intrinsic luminosity of Standard Candles? Intellectual Archive, September 2021. http://dx.doi.org/10.32370/iaj.2569.
Full text