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Journal articles on the topic 'Trappists'

Author: Grafiati

Published: 4 June 2021

Last updated: 30 July 2024

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1

Leach, Amy. "The Trappists." Iowa Review 36, no. 1 (2006): 55. http://dx.doi.org/10.17077/0021-065x.6167.

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2

Maltagliati, Luca. "Clouds over TRAPPISTs." Nature Astronomy 3, no. 1 (2018): 14. http://dx.doi.org/10.1038/s41550-018-0679-6.

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3

Khandlhela, Risimati Sam. "The Trappists in South Africa: a short overview." Kleio 27, no. 1 (1995): 46–62. http://dx.doi.org/10.1080/00232089585310041.

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4

Delpal, Bernard. "Travail, loisir et observance chez les trappistes au XIXe siècle / Work, Leisure and Observance among Trappists during the XIXth Century." Archives de sciences sociales des religions 86, no. 1 (1994): 213–33. http://dx.doi.org/10.3406/assr.1994.1440.

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5

Butler, Jay. "Agricultural Missionaries: The Trappists and French Colonial Policy under the July Monarchy." Catholic Historical Review 106, no. 2 (2020): 256–81. http://dx.doi.org/10.1353/cat.2020.0041.

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6

Balbo, Ned, and Richard Howard. "Trappings." Antioch Review 58, no. 3 (2000): 380. http://dx.doi.org/10.2307/4614044.

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7

Tan, Jin, and Ming-Fen Li. "Rapid and nondestructive identification of Belgian and Netherlandish Trappist beers by front-face synchronous fluorescence spectroscopy coupled with multiple statistical analysis." Quality Assurance and Safety of Crops & Foods 13, no. 1 (2021): 83–92. http://dx.doi.org/10.15586/qas.v13i1.839.

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Front-face synchronous fluorescence spectroscopy (FFSFS) was applied for the rapid and noninvasive recognition of Belgian and Netherlandish Trappist beers against non-Trappist beers. The front-face synchronous fluorescence spectra at wavelength intervals (??) of 30 and 60 nm for 80 bottles of beer, including 41 Trappist and 39 non-Trap-pist beers, were acquired in a 5 × 10 mm fused-quartz cuvette settled in a traditional right-angle sample compartment. The discrimination model was constructed by either principal component analysis (PCA) combined with linear discriminant analysis (LDA) or parti

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8

Maciel, Samara Rebeka Pita, and Jean Paulo dos Santos Carvalho. "Evolução Orbital dos Exoplanetas (TRAPPIST-1e e TRAPPIST-1g) que estão na Zona Habitável da Estrela TRAPPIST-1." Sitientibus Série Ciências Físicas 16 (December 30, 2020): 1. http://dx.doi.org/10.13102/sscf.v16i0.6010.

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A abordagem central baseia-se no problema de três corpos, em que é analisada a dinâmica secular de um sistema composto por uma estrela central e dois planetas sob influência gravitacional mútua, considerando a perturbação devido ao efeito da atração gravitacional do terceiro corpo em órbita elíptica e inclinada até a terceira ordem do potencial perturbador. Apresentamos uma análise da evolução orbital dos exoplanetas que estão na zona habitável da estrela. O software Maple é usado para fazer as integrações numéricas, outro software também utilizado é o Universe Sandbox para comparar o resultad

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Maciel, Samara Rebeka Pita, and Jean Paulo dos Santos Carvalho. "Evolução Orbital dos Exoplanetas (TRAPPIST-1e e TRAPPIST-1g) que estão na Zona Habitável da Estrela TRAPPIST-1." Sitientibus Série Ciências Físicas 16 (December 30, 2020): 1–13. http://dx.doi.org/10.13102/sscf.v16i.6010.

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A abordagem central baseia-se no problema de três corpos, em que é analisada a dinâmica secular de um sistema composto por uma estrela central e dois planetas sob influência gravitacional mútua, considerando a perturbação devido ao efeito da atração gravitacional do terceiro corpo em órbita elíptica e inclinada até a terceira ordem do potencial perturbador. Apresentamos uma análise da evolução orbital dos exoplanetas que estão na zona habitável da estrela. O software Maple é usado para fazer as integrações numéricas, outro software também utilizado é o Universe Sandbox para comparar o resultad

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10

Lienhard, F., D. Queloz, M. Gillon, et al. "Global analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey." Monthly Notices of the Royal Astronomical Society 497, no. 3 (2020): 3790–808. http://dx.doi.org/10.1093/mnras/staa2054.

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ABSTRACT We conducted a global analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey – a prototype of the SPECULOOS transit search conducted with the TRAPPIST-South robotic telescope in Chile from 2011 to 2017 – to estimate the occurrence rate of close-in planets such as TRAPPIST-1b orbiting ultra-cool dwarfs. For this purpose, the photometric data of 40 nearby ultra-cool dwarfs were reanalysed in a self-consistent and fully automated manner starting from the raw images. The pipeline developed specifically for this task generates differential light curves, removes non-planetary photometric

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11

Hochman, Assaf, Paolo De Luca, and Thaddeus D. Komacek. "Greater Climate Sensitivity and Variability on TRAPPIST-1e than Earth." Astrophysical Journal 938, no. 2 (2022): 114. http://dx.doi.org/10.3847/1538-4357/ac866f.

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Abstract The atmospheres of rocky exoplanets are close to being characterized by astronomical observations, in part due to the commissioning of the JWST. These observations compel us to understand exoplanetary atmospheres, in the voyage to find habitable planets. With this aim, we investigate the effect that CO2 partial pressure (pCO2) has on exoplanets’ climate variability, by analyzing results from ExoCAM model simulations of the tidally locked TRAPPIST-1e exoplanet, an Earth-like aqua-planet, and Earth itself. First, we relate the differences between the planets to their elementary paramete

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12

Bansal, Dhananjhay, Hannah S. Christie, and Mathieu Dumberry. "Libration- and Precession-driven Dissipation in the Fluid Cores of the TRAPPIST-1 Planets." Planetary Science Journal 4, no. 9 (2023): 171. http://dx.doi.org/10.3847/psj/acf3de.

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Abstract The seven planets orbiting TRAPPIST-1 have sizes and masses similar to Earth and mean densities that suggest that their interior structures are comprised of a fluid iron core and rocky mantle. Here we use idealized analytical models to compute estimates of the viscous dissipation in the fluid cores of the TRAPPIST-1 planets induced by mantle libration and precession. The dissipation induced by the libration at orbital periods is largest for TRAPPIST-1b, of the order of 600 MW, and decreases with orbital distance, to values of 5–500 W for TRAPPIST-1h, depending on its triaxial shape. E

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13

Teixeira, Katie E., Caroline V. Morley, Bradford J. Foley, and Cayman T. Unterborn. "The Carbon-deficient Evolution of TRAPPIST-1c." Astrophysical Journal 960, no. 1 (2023): 44. http://dx.doi.org/10.3847/1538-4357/ad0cec.

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Abstract Transiting planets orbiting M dwarfs provide the best opportunity to study the atmospheres of rocky planets with current facilities. As JWST enters its second year of science operations, an important initial endeavor is to determine whether these rocky planets have atmospheres at all. M dwarfs are thought to pose a major threat to planetary atmospheres due to their high magnetic activity over timescales of several billion years, and might completely strip atmospheres. Several Cycle 1 and 2 General Observers and Guaranteed Time Observations programs are testing this hypothesis, observi

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Turbet, Martin, Emeline Bolmont, Jeremy Leconte, et al. "Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets." Astronomy & Astrophysics 612 (April 2018): A86. http://dx.doi.org/10.1051/0004-6361/201731620.

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TRAPPIST-1 planets are invaluable for the study of comparative planetary science outside our solar system and possibly habitability. Both transit timing variations (TTV) of the planets and the compact, resonant architecture of the system suggest that TRAPPIST-1 planets could be endowed with various volatiles today. First, we derived from N-body simulations possible planetary evolution scenarios, and show that all the planets are likely in synchronous rotation. We then used a versatile 3D global climate model (GCM) to explore the possible climates of cool planets around cool stars, with a focus

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15

LIGO, Vivian. "The Trappist Monk Revisited." Louvain Studies 16, no. 4 (1991): 312–30. http://dx.doi.org/10.2143/ls.16.4.2013815.

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16

Bolmont, E., B. O. Demory, S. Blanco-Cuaresma, et al. "Impact of tides on the transit-timing fits to the TRAPPIST-1 system." Astronomy & Astrophysics 635 (March 2020): A117. http://dx.doi.org/10.1051/0004-6361/202037546.

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Transit timing variations (TTVs) can be a very efficient way of constraining masses and eccentricities of multi-planet systems. Recent measurements of the TTVs of TRAPPIST-1 have led to an estimate of the masses of the planets, enabling an estimate of their densities and their water content. A recent TTV analysis using data obtained in the past two years yields a 34 and 13% increase in mass for TRAPPIST-1b and c, respectively. In most studies to date, a Newtonian N-body model is used to fit the masses of the planets, while sometimes general relativity is accounted for. Using the Posidonius N-b

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17

Klopper, Abigail. "Gold trappings." Nature Physics 14, no. 7 (2018): 636. http://dx.doi.org/10.1038/s41567-018-0220-y.

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18

Grimm, Simon L., Brice-Olivier Demory, Michaël Gillon, et al. "The nature of the TRAPPIST-1 exoplanets." Astronomy & Astrophysics 613 (May 2018): A68. http://dx.doi.org/10.1051/0004-6361/201732233.

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Context. The TRAPPIST-1 system hosts seven Earth-sized, temperate exoplanets orbiting an ultra-cool dwarf star. As such, it represents a remarkable setting to study the formation and evolution of terrestrial planets that formed in the same protoplanetary disk. While the sizes of the TRAPPIST-1 planets are all known to better than 5% precision, their densities have significant uncertainties (between 28% and 95%) because of poor constraints on the planet’s masses. Aims. The goal of this paper is to improve our knowledge of the TRAPPIST-1 planetary masses and densities using transit-timing variat

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19

Lim, Olivia, Björn Benneke, René Doyon, et al. "Atmospheric Reconnaissance of TRAPPIST-1 b with JWST/NIRISS: Evidence for Strong Stellar Contamination in the Transmission Spectra." Astrophysical Journal Letters 955, no. 1 (2023): L22. http://dx.doi.org/10.3847/2041-8213/acf7c4.

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Abstract TRAPPIST-1 is a nearby system of seven Earth-sized, temperate, rocky exoplanets transiting a Jupiter-sized M8.5V star, ideally suited for in-depth atmospheric studies. Each TRAPPIST-1 planet has been observed in transmission both from space and from the ground, confidently rejecting cloud-free, hydrogen-rich atmospheres. Secondary eclipse observations of TRAPPIST-1 b with JWST/MIRI are consistent with little to no atmosphere given the lack of heat redistribution. Here we present the first transmission spectra of TRAPPIST-1 b obtained with JWST/NIRISS over two visits. The two transmiss

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20

Krissansen-Totton, Joshua. "Implications of Atmospheric Nondetections for Trappist-1 Inner Planets on Atmospheric Retention Prospects for Outer Planets." Astrophysical Journal Letters 951, no. 2 (2023): L39. http://dx.doi.org/10.3847/2041-8213/acdc26.

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Abstract JWST secondary eclipse observations of Trappist-1b seemingly disfavor atmospheres >∼1 bar since heat redistribution is expected to yield dayside emission temperature below the ∼500 K observed. Given the similar densities of Trappist-1 planets, and the theoretical potential for atmospheric erosion around late M dwarfs, this observation might be assumed to imply substantial atmospheres are also unlikely for the outer planets. However, the processes governing atmosphere erosion and replenishment are fundamentally different for inner and outer planets. Here, an atmosphere–interior evol

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21

Grootel, Valérie Van, Catarina S. Fernandes, Michael Gillon, et al. "Stellar Parameters for Trappist-1." Astrophysical Journal 853, no. 1 (2018): 30. http://dx.doi.org/10.3847/1538-4357/aaa023.

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22

Dmitrienko, E. S., and I. S. Savanov. "Activity of TRAPPIST-1 Analogs." Astronomy Letters 48, no. 11 (2022): 676–81. http://dx.doi.org/10.1134/s1063773722110068.

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23

Hammond, Tobi, and Thaddeus D. Komacek. "The Coupled Impacts of Atmospheric Composition and Obliquity on the Climate Dynamics of TRAPPIST-1e." Astrophysical Journal 968, no. 1 (2024): 43. http://dx.doi.org/10.3847/1538-4357/ad4a59.

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Abstract Planets in multiplanet systems are expected to migrate inward as near-resonant chains, thus allowing them to undergo gravitational planet–planet interactions and possibly maintain a nonzero obliquity. The TRAPPIST-1 system is in such a near-resonant configuration, making it plausible that TRAPPIST-1e has a nonzero obliquity. In this work, we use the ExoCAM general circulation model to study the possible climates of TRAPPIST-1e at varying obliquities and atmospheric compositions. We vary obliquity from 0° to 90° and the partial pressure of carbon dioxide from 0.0004 bar (modern Earth-l

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24

Gialluca, Megan T., Rory Barnes, Victoria S. Meadows, Rodolfo Garcia, Jessica Birky, and Eric Agol. "The Implications of Thermal Hydrodynamic Atmospheric Escape on the TRAPPIST-1 Planets." Planetary Science Journal 5, no. 6 (2024): 137. http://dx.doi.org/10.3847/psj/ad4454.

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Abstract JWST observations of the seven-planet TRAPPIST-1 system will provide an excellent opportunity to test outcomes of stellar-driven evolution of terrestrial planetary atmospheres, including atmospheric escape, ocean loss, and abiotic oxygen production. While most previous studies use a single luminosity evolution for the host star, we incorporate observational uncertainties in stellar mass, luminosity evolution, system age, and planetary parameters to statistically explore the plausible range of planetary atmospheric escape outcomes. We present probabilistic distributions of total water

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25

Gressier, A., M. Mori, Q. Changeat, et al. "Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations." Astronomy & Astrophysics 658 (February 2022): A133. http://dx.doi.org/10.1051/0004-6361/202142140.

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Context. The TRAPPIST-1 planetary system is favourable for transmission spectroscopy and offers the unique opportunity to study rocky planets with possibly non-primary envelopes. We present here the transmission spectrum of the seventh planet of the TRAPPIST-1 system, TRAPPIST-1 h (RP = 0.752 R⊕, Teq = 173 K) using Hubble Space Telescope (HST), Wide Field Camera 3 Grism 141 (WFC3/G141) data. Aims. Our purpose is to reduce the HST observations of the seventh planet of the TRAPPIST-1 system and, by testing a simple atmospheric hypothesis, to put a new constraint on the composition and the nature

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KOVINCIC, IVANA, IVICA F. VUJICIC, MELINA SVABIC-VLAHOVIC, MIRJANA VULIC, MAJA GAGIC, and IRENE V. WESLEY. "Survival of Listeria monocytogenes During the Manufacture and Ripening of Trappist Cheese." Journal of Food Protection 54, no. 6 (1991): 418–20. http://dx.doi.org/10.4315/0362-028x-54.6.418.

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Trappist cheese constitutes more than one-third of the semisoft cheese production in Yugoslavia. The ability of Listeria monocytogenes to survive the Trappist cheese-making process and persist during 90 d of ripening and storage was examined. Trappist cheese was manufactured from pasteurized milk (trials A, B, C) and from whey (trials D and E) inoculated with L. monocytogenes (2.46–5.38 log10 CFU/ml). An increase in L. monocytogenes counts was detected after 30 d of ripening in all of the five trials. After ripening and storage for 90 d, the L. monocytogenes counts ranged from 2.72–5.64 log10

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27

Lin, Zifan, Ryan J. MacDonald, Lisa Kaltenegger, and David J. Wilson. "Differentiating modern and prebiotic Earth scenarios for TRAPPIST-1e: high-resolution transmission spectra and predictions for JWST." Monthly Notices of the Royal Astronomical Society 505, no. 3 (2021): 3562–78. http://dx.doi.org/10.1093/mnras/stab1486.

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ABSTRACT The TRAPPIST-1 system is a priority target for terrestrial exoplanet characterization. TRAPPIST-1e, residing in the habitable zone, will be observed during the James Webb Space Telescope (JWST) GTO Program. Here, we assess the prospects of differentiating between prebiotic and modern Earth scenarios for TRAPPIST-1e via transmission spectroscopy. Using updated TRAPPIST-1 stellar models from the Mega-MUSCLES survey, we compute self-consistent model atmospheres for a 1 bar prebiotic Earth scenario and two modern Earth scenarios (1 and 0.5 bar eroded atmosphere). Our modern and prebiotic

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28

Ogihara, Masahiro, Eiichiro Kokubo, Ryuunosuke Nakano, and Takeru K. Suzuki. "Rapid-then-slow migration reproduces mass distribution of TRAPPIST-1 system." Astronomy & Astrophysics 658 (February 2022): A184. http://dx.doi.org/10.1051/0004-6361/202142354.

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Context. The TRAPPIST-1 system is an iconic planetary system in various aspects (e.g., habitability, resonant relation, and multiplicity) and hence has attracted considerable attention. The mass distribution of the TRAPPIST-1 planets is characterized by two features: the two inner planets are large, and the masses of the four planets in the outer orbit increase with orbital distance. The origin of these features cannot be explained by previous formation models. Aims. We investigate whether the mass distribution of the TRAPPIST-1 system can be reproduced by a planet formation model using N-body

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29

Đošović, Vladimir, Bojan Novakovć, Branislav Vukotć, and Milan M. Ćirković. "Water transport throughout the TRAPPIST-1 system: the role of planetesimals." Monthly Notices of the Royal Astronomical Society 499, no. 4 (2020): 4626–37. http://dx.doi.org/10.1093/mnras/staa1833.

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ABSTRACT Observational data suggest that a belt of planetesimals is expected close to the snow line in protoplanetary discs. Assuming there is such a belt in the TRAPPIST-1 system, we examine possibilities of water delivery to the planets via planetesimals from the belt. The study is accomplished by numerical simulations of dynamical evolution of a hypothetical planetesimal belt. Our results show that the inner part of the belt is dynamically unstable and planetesimals located in this region are quickly scattered away, with many of them entering the region around the planets. The main dynamica

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30

Basant, Ritvik, Jeremy Dietrich, and Dániel Apai. "Prediction of an Earth-sized Planet Formed in the Habitable Zone of the SPECULOOS-2 System." Research Notes of the AAS 6, no. 10 (2022): 213. http://dx.doi.org/10.3847/2515-5172/ac9ab8.

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Abstract Transiting planets in the nearby TRAPPIST-1 system provide rare examples of habitable zone (HZ), Earth-sized planets that can be characterized via transmission spectroscopy. However, these present-day HZ planets likely formed interior to HZ and probably underwent an evolution very different from that of Earth. We present the integrative analysis of the planetary architecture of the recently discovered planetary system SPECULOOS-2. Our analysis answers the question: If there are additional exoplanets in the SPECULOOS-2 system, what are their orbital and physical properties? We predict

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31

Christodoulou, Dimitris M., and Demosthenes Kazanas. "Predicting Additional Planets in TRAPPIST-1." Research Notes of the AAS 3, no. 3 (2019): 50. http://dx.doi.org/10.3847/2515-5172/ab0e13.

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32

Morris, Brett M., Eric Agol, James R. A. Davenport, and Suzanne L. Hawley. "Possible Bright Starspots on TRAPPIST-1." Astrophysical Journal 857, no. 1 (2018): 39. http://dx.doi.org/10.3847/1538-4357/aab6a5.

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Maltagliati, Luca. "Investigating TRAPPIST-1 e atmospheric scenarios." Nature Astronomy 5, no. 6 (2021): 530. http://dx.doi.org/10.1038/s41550-021-01410-3.

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Hay, Hamish C. F. C., and Isamu Matsuyama. "Tides Between the TRAPPIST-1 Planets." Astrophysical Journal 875, no. 1 (2019): 22. http://dx.doi.org/10.3847/1538-4357/ab0c21.

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35

Kipping, David. "Predicting The Orbit of TRAPPIST-1i." Research Notes of the AAS 2, no. 3 (2018): 136. http://dx.doi.org/10.3847/2515-5172/aad6e8.

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36

Tarr, Kathleen. "The Trappist Monk and Pasternak's Tree." Sewanee Review 121, no. 3 (2013): 449–59. http://dx.doi.org/10.1353/sew.2013.0062.

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Dong, Chuanfei, Meng Jin, Manasvi Lingam, Vladimir S. Airapetian, Yingjuan Ma, and Bart van der Holst. "Atmospheric escape from the TRAPPIST-1 planets and implications for habitability." Proceedings of the National Academy of Sciences 115, no. 2 (2017): 260–65. http://dx.doi.org/10.1073/pnas.1708010115.

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The presence of an atmosphere over sufficiently long timescales is widely perceived as one of the most prominent criteria associated with planetary surface habitability. We address the crucial question of whether the seven Earth-sized planets transiting the recently discovered ultracool dwarf star TRAPPIST-1 are capable of retaining their atmospheres. To this effect, we carry out numerical simulations to characterize the stellar wind of TRAPPIST-1 and the atmospheric ion escape rates for all of the seven planets. We also estimate the escape rates analytically and demonstrate that they are in g

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Mandt, Kathleen, Adrienn Luspay-Kuti, Jacob Lustig-Yaeger, Ryan Felton, and Shawn Domagal-Goldman. "TRAPPIST-1h as an Exo-Titan. I. The Role of Assumptions about Atmospheric Parameters in Understanding an Exoplanet Atmosphere." Astrophysical Journal 930, no. 1 (2022): 73. http://dx.doi.org/10.3847/1538-4357/ac59bb.

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Abstract The TRAPPIST-1 system is home to at least seven terrestrial planets and is a target of interest for future James Webb Space Telescope (JWST) observations. Additionally, these planets will be of interest to future missions making observations in the ultraviolet (UV). Although several of these planets are located in the traditional habitable zone, where liquid water could exist on the surface, TRAPPIST-1h is interesting to explore as a potentially habitable ocean world analog. In this study, we evaluate the observability of a Titan-like atmosphere on TRAPPIST-1h. The ability of the JWST

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Myttenaere, Bernard De. "Valorisation touristique des bières trappistes en Wallonie." Mondes du tourisme, no. 7 (June 1, 2013): 68–83. http://dx.doi.org/10.4000/tourisme.186.

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Soung Yee, L., P. Álvarez, E. Martin, E. Cortina, and C. Ferrer. "Test of the TRAPPISTe monolithic detector system." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 731 (December 2013): 141–45. http://dx.doi.org/10.1016/j.nima.2013.03.052.

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Cortina, E., L. Soung Yee, C. Renaux, D. Flandre та E. Martin. "TRAPPISTe pixel sensor with 2μm SOI technology". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 633 (травень 2011): S19—S21. http://dx.doi.org/10.1016/j.nima.2010.06.109.

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42

Quinn, Justin, Tim Kendall, Richard Kirkland, and Luke Gibbons. "The Trappings of Politics." Irish Review (1986-), no. 21 (1997): 159. http://dx.doi.org/10.2307/29735877.

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Oenbring, Raymond, and Matthias Klumm. "The trappings of order." English World-Wide 43, no. 1 (2021): 66–95. http://dx.doi.org/10.1075/eww.21020.oen.

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Abstract This study builds off of previous research into Caribbean Standard Englishes (which has largely used newspaper genres) by comparing the rates of features found in corpora of Bahamian, Jamaican, British, and American administrative writing, paying particular attention to whether and how the noted formality of Caribbean Standard Englishes manifests itself in administrative writing. The study employs expanded versions of ICE administrative subcorpora for the analysis. Features analyzed include lexis, orthography, as well as different morphosyntactic constructions such as be-passives and

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Martin, John Frederick. "The Trappings of Democracy." Historically Speaking 14, no. 4 (2013): 2–7. http://dx.doi.org/10.1353/hsp.2013.0039.

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Brewer, Paul R. "The Trappings of Science." Science Communication 35, no. 3 (2012): 311–33. http://dx.doi.org/10.1177/1075547012454599.

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Grier, David Alan. "The Trappings of Power." Computer 46, no. 11 (2013): 120. http://dx.doi.org/10.1109/mc.2013.399.

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Brain, J. B. "Mariannhill monastery, 1882-1982." New Contree 13 (July 11, 2024): 5. http://dx.doi.org/10.4102/nc.v13i0.785.

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The Mariannhill monastery was established in 1882 on the farm Zeekoegat in Natal by the Trappist monks who, before any direct evangelization, cultivated the large and productive monastery farm and erected the necessary buildings. Formal mission work did not begin until 1884 and by 1898, with 185 monks, Mariannhill had become the largest abbey in the world. It was separated in 1909 from the Trappist order and became a separate missionary congregation known as the Congregation of Missionaries of Mariannhill. Today Mariannhill missionaries are at work not only in Natal, but also in the Transkei,

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Turbet, Martin, Thomas J. Fauchez, Denis E. Sergeev, et al. "The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI). I. Dry Cases—The Fellowship of the GCMs." Planetary Science Journal 3, no. 9 (2022): 211. http://dx.doi.org/10.3847/psj/ac6cf0.

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Abstract With the commissioning of powerful, new-generation telescopes such as the James Webb Space Telescope (JWST) and the ground-based Extremely Large Telescopes, the first characterization of a high molecular weight atmosphere around a temperate rocky exoplanet is imminent. Atmospheric simulations and synthetic observables of target exoplanets are essential to prepare and interpret these observations. Here we report the results of the first part of the TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) project, which compares 3D numerical simulations performed with four state-of-the-ar

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49

Howard, Ward S., Adam F. Kowalski, Laura Flagg, et al. "Characterizing the Near-infrared Spectra of Flares from TRAPPIST-1 during JWST Transit Spectroscopy Observations." Astrophysical Journal 959, no. 1 (2023): 64. http://dx.doi.org/10.3847/1538-4357/acfe75.

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Abstract We present the first analysis of JWST near-infrared spectroscopy of stellar flares from TRAPPIST-1 during transits of rocky exoplanets. Four flares were observed from 0.6–2.8 μm with the Near Infrared Imager and Slitless Spectrograph and 0.6–3.5 μm with the Near Infrared Spectrograph during transits of TRAPPIST-1b, f, and g. We discover Pα and Brβ line emission and characterize flare continuum at wavelengths from 1–3.5 μm for the first time. Observed lines include Hα, Pα–Pϵ, Brβ, He i λ0.7062 μm, two Ca ii infrared triplet (IRT) lines, and the He i IRT. We observe a reversed Paschen d

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50

Davoudi, Fatemeh, Benjamin V. Rackham, Michaël Gillon, et al. "Updated Spectral Characteristics for the Ultracool Dwarf TRAPPIST-1." Astrophysical Journal Letters 970, no. 1 (2024): L4. http://dx.doi.org/10.3847/2041-8213/ad5c6c.

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Abstract A comprehensive infrared spectroscopic study of star TRAPPIST-1 is a crucial step toward the detailed examination of its planets. While the presence of Earth’s atmosphere has limited the spectral extent of such a study up to now, the Near Infrared Imager and Slitless Spectrograph (NIRISS) and the Near Infrared Spectrograph instruments aboard the James Webb Space Telescope (JWST) can now yield the 0.6–5 μm spectral energy distribution (SED) of the star. Here we translate TRAPPIST-1's SED into tight constraints on its luminosity (L bol = 0.000566 ± 0.000022 L ⊙), effective temperature (

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