exoplanet diversity — SPP 1992 – The DFG SPP “Exploring the Diversity of Extrasolar Planets” (2024)

E. W. Guenther, E. Goffo, D. Sebastian, A. M. S. Smith, C. M. Persson, M. Fridlund, D. Gandolfi, J. Korth

A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c

bib

@misc{guenther2024new,
title={A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c},
author={E. W. Guenther and E. Goffo and D. Sebastian and A. M. S. Smith and C. M. Persson and M. Fridlund and D. Gandolfi and J. Korth},
year={2024},
eprint={2402.09322},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

arXiv

L. M. Bernabò, Sz. Csizmadia, A. M. S. Smith, H. Rauer, A. P. Hatzes, M. Esposito, D. Gandolfi, J. Cabrera

Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system

bib

@article{Bernabo_2024,
title={Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system},
ISSN={1432-0746},
url={http://dx.doi.org/10.1051/0004-6361/202346852},
DOI={10.1051/0004-6361/202346852},
journal={Astronomy & Astrophysics},
publisher={EDP Sciences},
author={Bernabo, L.M. and Csizmadia, Sz. and Smith, A.M.S. and Rauer, H. and Hatzes, A. and Esposito, M. and Gandolfi, D. and Cabrera, J.},
year={2024},
month=jan }

DOI arXiv

B. Akinsanmi, S. C. C. Barros, M. Lendl, L. Carone, P. E. Cubillos, A. Bekkelien, A. Fortier, H. -G. Florén, A. Collier Cameron, G. Boué, G. Bruno, B. O. Demory, A. Brandeker, S. G. Sousa, T. G. Wilson, A. Deline, A. Bonfanti, G. Scandariato, M. J. Hooton, A. C. M. Correia, O. D. S. Demangeon, A. M. S. Smith, V. Singh, Y. Alibert, R. Alonso, J. Asquier,, T. Bárczy, D. Barrado Navascues, W. Baumjohann, M. Beck, T. Beck, W. Benz, N. Billot, X. Bonfils, L. Borsato, C. Broeg, M. Buder, S. Charnoz, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, D. Ehrenreich, A. Erikson, J. Farinato, L. Fossati, M. C. V. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, M. N. Guenther, A. Heitzmann, Ch. Helling, S. Hoyer, K. G. Isaak, L. Kiss, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, D. Magrin, P. F. L. Maxted, M. Mecina, C. Mordasini, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, N. C. Santos, D. Ségransan, A. E. Simon, M. Stalport, G. M. Szabó, N. Thomas, S. Udry, V. Van Grootel, J. Venturini, E. Villaver, N. A. Walton

The tidal deformation and atmosphere of WASP-12b from its phase curve

bib

@misc{akinsanmi2024tidal,
title={The tidal deformation and atmosphere of WASP-12b from its phase curve},
author={B. Akinsanmi and S. C. C. Barros and M. Lendl and L. Carone and P. E. Cubillos and A. Bekkelien and A. Fortier and H. -G. Florén and A. Collier Cameron and G. Boué and G. Bruno and B. -O. Demory and A. Brandeker and S. G. Sousa and T. G. Wilson and A. Deline and A. Bonfanti and G. Scandariato and M. J. Hooton and A. C. M. Correia and O. D. S. Demangeon and A. M. S. Smith and V. Singh and Y. Alibert and R. Alonso and J. Asquier and T. Bárczy and D. Barrado Navascues and W. Baumjohann and M. Beck and T. Beck and W. Benz and N. Billot and X. Bonfils and L. Borsato and Ch. Broeg and M. Buder and S. Charnoz and Sz. Csizmadia and M. B. Davies and M. Deleuil and L. Delrez and D. Ehrenreich and A. Erikson and J. Farinato and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and A. Heitzmann and Ch. Helling and S. Hoyer and K. G. Isaak and L. L. Kiss and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and D. Magrin and P. F. L. Maxted and M. Mecina and Ch. Mordasini and V. Nascimbeni and G. Olofsson and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and D. Piazza and G. Piotto and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and N. C. Santos and D. Ségransan and A. E. Simon and M. Stalport and Gy. M. Szabó and N. Thomas and S. Udry and V. Van Grootel and J. Venturini and E. Villaver and N. A. Walton},
year={2024},
eprint={2402.10486},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

arXiv

exoplanet diversity — SPP 1992 – The DFG SPP “Exploring the Diversity of Extrasolar Planets” (2024)

FAQs

What exoplanet was discovered in 1992? ›

The first exoplanet was discovered in 1992. In fact, the first discovery wasn't just 1 planet it was 2! Poltergeist and Phobetor were found orbiting a pulsar called PSR B1257+12.

How many extrasolar planets have been detected since 1995? ›

Detection Methods. Swiss astronomers Michael Mayor and Didier Queloz discovered the first exoplanet in 1995. Since then, the number of verified exoplanets has surpassed 200.

What is an extrasolar planet group of answer choices? ›

extrasolar planet, any planetary body that is outside the solar system and that usually orbits a star other than the Sun. Extrasolar planets were first discovered in 1992. More than 5,000 are known, and almost 9,000 await further confirmation.

What is an extrasolar planet Quizlet? ›

What is an extrasolar planet? A planet that orbits a star that is not our own Sun. ("Extrasolar" means "beyond the Sun.")

What did the first exoplanet teach us? ›

Mayor and Queloz found the first exoplanet orbiting a sunlike star, which was a landmark discovery for two reasons: it showed conclusively that the sun isn't the only star to host a family of planets (something we had long figured but never demonstrated), and also that the universe is really, really weird.

What was the first real image of an exoplanet? ›

This composite image shows an exoplanet (the red spot on the lower left), orbiting the brown dwarf 2M1207 (centre). 2M1207b is the first exoplanet directly imaged and the first discovered orbiting a brown dwarf. It was imaged the first time by the VLT in 2004.

Is Earth an exoplanet? ›

No earth is not an exoplanet but a terrestrial planet. Earth has a solid, rocky, and very active surface that has plains, canyons, valleys, and mountains among other features.

How many exoplanets exist? ›

To date, more than 5,000 exoplanets have been discovered and are considered "confirmed" out of the billions in our galaxy alone. There are thousands of other "candidate" exoplanet detections that require further observations in order to say for sure whether or not the exoplanet is real.

Why is Pluto not a planet? ›

According to the IAU, Pluto is technically a “dwarf planet,” because it has not “cleared its neighboring region of other objects.” This means that Pluto still has lots of asteroids and other space rocks along its flight path, rather than having absorbed them over time, like the larger planets have done.

Why are exoplanets called exoplanets? ›

The prefix exo is short for extrasolar, meaning beyond the Sun, so exoplanets are just planets that orbit stars other than our Sun.

Is an exoplanet considered a planet? ›

Planets that orbit around other stars are called exoplanets. All of the planets in our solar system orbit around the Sun. Planets that orbit around other stars are called exoplanets. Exoplanets are very hard to see directly with telescopes.

What are the 4 exoplanets? ›

So far scientists have categorized exoplanets into the following types: Gas giant, Neptunian, super-Earth and terrestrial.

Are extrasolar and exoplanets the same? ›

SUMMARY: An extrasolar planet, or exoplanet, is a planet outside of our solar system that orbits a star other than our Sun.

What is an exoplanet defined to be ____________? ›

An exoplanet is a planet that is located outside our Solar System. While there is currently no formal agreement on what exactly defines an exoplanet, the word is used to indicate planet-sized bodies that are located beyond our Solar System.

What are extrasolar planets made of? ›

Exoplanets are made up of elements similar to that of the planets in our solar system, but their mixes of those elements may differ. Some planets may be dominated by water or ice, while others are dominated by iron or carbon.

What planet was discovered in 1993? ›

(181708) 1993 FW (provisional designation 1993 FW) is a cubewano and was the second trans-Neptunian object to be discovered after Pluto and Charon, the first having been 15760 Albion, formerly known as (15760) 1992 QB1. It was discovered in 1993 by David C. Jewitt and Jane X.

Who discovered planet GJ 504b? ›

Gliese 504 b
Discovery
Discovered byKuzuhara et al.
Discovery siteSubaru Telescope
Discovery date2013
Detection methodDirect imaging
17 more rows

When was Kepler 452b discovered? ›

The Kepler space telescope identified the exoplanet, and its discovery was announced by NASA on 23 July 2015. The planet is about 1,800 light-years (550 pc) away from the Solar System.

Is TOI-715 b habitable? ›

TOI-715 b is a super-Earth exoplanet in the habitable zone of its parent M-type star, TOI-715. The planet is 1.55 times larger than Earth, and is located at 0.083 astronomical units (12,400,000 km) from its star. The planet orbits on the habitable zone of its star and has an equilibrium temperature of 234 K (−39 °C).

References

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