Detection and characterization of an ultra-dense sub-Neptunian planet orbiting the Sun-like star K2-292★

Astronomy & Astrophysics EDP Sciences 623 (2019) a114

Authors:

R Luque, G Nowak, E Pallé, F Dai, A Kaminski, E Nagel, D Hidalgo, F Bauer, M Lafarga, J Livingston, O Barragán, T Hirano, M Fridlund, D Gandolfi, AB Justesen, M Hjorth, V Van Eylen, JN Winn, M Esposito, JC Morales, S Albrecht, R Alonso, PJ Amado, P Beck, JA Caballero, J Cabrera, WD Cochran, Sz Csizmadia, H Deeg, Ph Eigmüller, M Endl, A Erikson, A Fukui, S Grziwa, EW Guenther, AP Hatzes, E Knudstrup, J Korth, KWF Lam, MN Lund, S Mathur, P Montañes-Rodríguez, N Narita, D Nespral, P Niraula, M Pätzold, CM Persson, J Prieto-Arranz, A Quirrenbach, H Rauer, S Redfield, A Reiners, I Ribas, AMS Smith

HD 219666 b: a hot-Neptune from TESS Sector 1★

Astronomy & Astrophysics EDP Sciences 623 (2019) a165

Authors:

M Esposito, DJ Armstrong, D Gandolfi, V Adibekyan, M Fridlund, NC Santos, JH Livingston, E Delgado Mena, L Fossati, J Lillo-Box, O Barragán, D Barrado, PE Cubillos, B Cooke, AB Justesen, F Meru, RF Díaz, F Dai, LD Nielsen, CM Persson, PJ Wheatley, AP Hatzes, V Van Eylen, MM Musso, R Alonso, PG Beck, SCC Barros, D Bayliss, AS Bonomo, F Bouchy, DJA Brown, E Bryant, J Cabrera, WD Cochran, S Csizmadia, H Deeg, O Demangeon, M Deleuil, X Dumusque, P Eigmüller, M Endl, A Erikson, F Faedi, P Figueira, A Fukui, S Grziwa, EW Guenther, D Hidalgo, M Hjorth, T Hirano, S Hojjatpanah, E Knudstrup, J Korth, KWF Lam, J de Leon, MN Lund, R Luque, S Mathur, P Montañés Rodríguez, N Narita, D Nespral, P Niraula, G Nowak, HP Osborn, E Pallé, M Pätzold, D Pollacco, J Prieto-Arranz, H Rauer, S Redfield, I Ribas, SG Sousa, AMS Smith, M Tala-Pinto, S Udry, JN Winn

Climate impacts of cultured meat and beef cattle

Frontiers in Sustainable Food Systems Frontiers Media 3 (2019) 5

Authors:

John Lynch, Raymond Pierrehumbert

Abstract:

Improved greenhouse gas (GHG) emission efficiency of production has been proposed as one of the biggest potential advantages of cultured meat over conventional livestock production systems. Comparisons with beef are typically highlighted, as it is a highly emissions intensive food product. In this study, we present a more rigorous comparison of the potential climate impacts of cultured meat and cattle production than has previously been made. Warming impacts are evaluated using a simple climate model that simulates the different behaviors of carbon dioxide (CO2), methane (CH4), and nitrous oxide (N2O), rather than relying on carbon dioxide equivalent (CO2e) metrics. We compare the temperature impact of beef cattle and cultured meat production at all times to 1,000 years in the future, using four synthetic meat GHG footprints currently available in the literature and three different beef production systems studied in an earlier climate modeling paper. Cattle systems are associated with the production of all three GHGs above, including significant emissions of CH4, while cultured meat emissions are almost entirely CO2 from energy generation. Under continuous high global consumption, cultured meat results in less warming than cattle initially, but this gap narrows in the long term and in some cases cattle production causes far less warming, as CH4 emissions do not accumulate, unlike CO2. We then model a decline in meat consumption to more sustainable levels following high consumption, and show that although cattle systems generally result in greater peak warming than cultured meat, the warming effect declines and stabilizes under the new emission rates of cattle systems, while the CO2 based warming from cultured meat persists and accumulates even under reduced consumption, again overtaking cattle production in some scenarios. We conclude that cultured meat is not prima facie climatically superior to cattle; its relative impact instead depends on the availability of decarbonized energy generation and the specific production systems that are realized.

Gas Jet Morphology and the Very Rapidly Increasing Rotation Period of Comet 41P/Tuttle–Giacobini–Kresák

The Astronomical Journal, Volume 157, Number 3

Authors:

David G. Schleicher, Matthew M. Knight, Nora L. Eisner and Audrey Thirouin

Abstract:

We present results from our 47 night imaging campaign of Comet 41P/Tuttle–Giacobini–Kresák conducted from Lowell Observatory between 2017 February 16 and July 2. Coma morphology revealed gas jets, whose appearance and motion as a function of time yielded the rotation period and other properties. All narrowband CN images exhibited either one or two jets; one jet appeared as a partial face-on spiral with clockwise rotation, while the second jet evolved from a side-on corkscrew, through face-on, to corkscrew again, with only a slow evolution throughout the apparition due to progressive viewing geometry changes. A total of 78 period determinations were made over a 7 week interval, yielding a smooth and accelerating rotation period starting at 24 hr (March 21 and 22) and passing 48 hr on April 28. While this is by far the fastest rate of change ever measured for a comet nucleus, the torque required is readily within what can exist given likely properties of the nucleus. If the torque remained constant, we estimate that the nucleus could have stopped rotating and/or begun to tumble as soon as only 2 months following perihelion and will certainly reach this stage by early in the next apparition. Working backward in time, Tuttle–Giacobini–Kresák would have been rotating near its rotational breakup velocity three to four orbits earlier, suggesting that its extreme 7 mag outburst observed in 2001 might have been caused by a partial fragmentation at that time, as might the pair of 1973 8 mag outbursts if there had been an earlier spin-down and spin-up cycle.

Oxidised micrometeorites as evidence for low atmospheric pressure on the early Earth

Geochemical Perspectives Letters European Association of Geochemistry (2019) 38-42

Authors:

PB Rimmer, O Shorttle, S Rugheimer