Astro Vol.12 Issue 8

Total Page:16

File Type:pdf, Size:1020Kb

Astro Vol.12 Issue 8 “It has become appallingly obvious that our technology has exceeded our humanity.” Albert Einstein ASTRONEWSLETTER Volume 12, Issue 8 May 31, 2019 CONTENTS • NASA Invites Public to Submit Names to Fly Aboard Next Mars Rover ...................1 • SpaceX Launched Its Starlink Satellites ..................1 • The ‘Forbidden’ Planet Has Been Found ................. 2 • Rare Meteorites Found in Costa Rica ....................2 • New Way to Make Breathable Oxygen on Mars .............3 • Strange Martian Mineral . 3 NASA Invites Public to Submit Names to Fly Aboard Next Mars Rover Although it will be years before the first humans set foot on Mars, NASA is giving the public an opportunity to send their names — stenciled on chips — to the Red SpaceX Launched Its Planet with NASA’s Mars 2020 rover, which represents the initial leg of humanity’s first round trip to another planet. The Starlink Satellites rover is scheduled to launch as early as July 2020, with the spacecraft expected After several delays, SpaceX has finally launched the first 60 satellites of its Starlink to touch down on Mars in February 2021. program. The California company hopes that the satellites, launched on a Falcon The opportunity to send your name to 9 rocket whose booster was making its third mission, will eventually be joined Mars comes with a souvenir boarding pass by 12,000 or so others as the company attempts to expand low-cost broadband and “frequent flyer” points. More than 2 million names flew on NASA’s InSight internet across the globe. mission to Mars, giving each “flyer” about 300 million frequent flyer miles (nearly 500 million frequent flyer kilometers). The Falcon 9 rocket’s booster successfully landed on the company’s “Of Course I Still Love You” droneship, stationed in the Atlantic Ocean. The landing marked From now until Sept. 30, you can add your name to the list and obtain a souvenir SpaceX’s 40th successful booster recovery. PopularMechanics.com boarding pass to Mars here: https://go.nasa.gov/Mars2020Pass Astro Newsletter 1 NASA.gov The ‘Forbidden’ Planet Has Been Found in the ‘Neptunian Desert’ The ‘Forbidden’ Planet Has Been Found in the Rare Meteorites Found in Costa Rica ‘Neptunian Desert’ Could Shed Light on Earth’s Water An exoplanet smaller than Neptune with its own atmosphere has been discovered in Meteorites are an astronomer’s carbonaceous chondrites can make the Neptunian Desert, by an international dream. In a field that by definition them surprisingly fragile once they collaboration of astronomers, with the studies objects and phenomena hit the ground. They’re basically University of Warwick taking a leading above and beyond Earth’s balls of clay, and dissolve rapidly atmosphere, many researchers when exposed to more water – role. New research, led by Dr. Richard West never get a chance to touch or see and May marks the beginning of including Professor Peter Wheatley, Dr. up close the things they study. the rainy season in Costa Rica. So Daniel Bayliss and Dr. James McCormac But then, sometimes, these items meteorite hunters knew there was from the Astronomy and Astrophysics simply rain down from the sky, in a clock ticking as soon as the fireball Group at the University of Warwick, the form of ancient space rocks streaked across the skies above has identified a rogue planet. NGTS called meteorites. Meteorites come Aguas Zarcas. is situated at the European Southern in many different types. But some Observatory’s Paranal Observatory in the of the most precious are called They ended up having five days to heart of the Atacama Desert, Chile. It is carbonaceous chondrites, valued search for and collect the meteorites a collaboration between UK Universities because they contain large amounts from the surrounding area before of water and organic compounds. the rain fell. About 55 pounds have Warwick, Leicester, Cambridge, and These meteorites contain a history been collected so far. Some of Queen’s University Belfast, together with of that water from the solar system’s them have made their way to ASU Observatoire de Genève, DLR Berlin and early days, and trace how the thanks to a meteorite hunter named Universidad de Chile. materials of life were distributed Michael Farmer. He collected some across the planets and space. of the space rocks or bought them Dr. Richard West, from the Department from locals and donated them to of Physics at the University of Warwick On April 23 of this year, one of ASU, which has a dedicated Center comments: these space rocks – roughly the size for Meteorite Studies. Researchers of a washing machine – streaked there are comparing the Aguas “This planet must be tough—it is right in through the skies over the Costa Zarcas fall to other, previously Rican town of Aguas Zarcas. As known meteorites so they can the zone where we expected Neptune- it fell, it broke into many smaller be more accurately classified. All sized planets could not survive. It is truly pieces, and astronomers scrambled meteorites began as part of larger remarkable that we found a transiting to collect and study them. They are asteroids. These building blocks of planet via a star dimming by less than the first large fall of carbonaceous the solar system are the same as the 0.2% - this has never been done before chondrites in half a century, and long-ago space rocks that collided by telescopes on the ground, and it was should provide ample data on the to form Earth and the other planets, great to find after working on this project history of water in the solar system, and could be the source of Earth’s for a year. according to a press release from water and other materials vital for Arizona State University, which is the formation of life. By analyzing studying the meteorites. the detailed chemistry of the water “We are now scouring out data to see if we contained in meteorites, researchers can see any more planets in the Neptune Mud balls can learn when and how Earth Desert—perhaps the desert is greener Even though meteoroids have obtained its water, which had a big than was once thought.” survived in space for billions of impact on Earth’s early history. Phys.org years, all the water contained in 2 Astro Newsletter Astronomy.com Scientists Cook Up a New Way to Make Breathable Oxygen on Mars Strange Martian Mineral Scientists Cook Up a New Way to Deposit Likely Sourced From Volcanic Explosions Make Breathable Oxygen on Mars Ashfall from ancient volcanic explosions Scientists have found a new way Molecular oxygen can also be is the likely source of a strange mineral that future Mars explorers could produced through carbon dioxide deposit near the landing site for NASA’s potentially generate their own reactions, the team found. (Carbon next Mars rover, a new study finds. The oxygen. Mars is a long way from dioxide contains a single carbon research, published in the journal Geology, Earth, so being able to create atom and two oxygen atoms.) could help scientists assemble a timeline breathable air on-site would save Former Caltech postdoctoral fellow of volcanic activity and environmental money and effort in having to haul Yunxi Yao and current Caltech conditions on early Mars. oxygen all the way from our own chemical engineering professor planet. A research team discovered Konstantinos Giapis simulated “This is one of the most tangible pieces of this new oxygen-generating this reaction by crashing carbon evidence yet for the idea that explosive reaction by studying comets. Most dioxide into gold foil. Since gold volcanism was more common on early of these small icy worlds originate foil cannot be oxidized, by itself it Mars,” said Christopher Kremer, a graduate in a distant area of the solar system should not produce any molecular student at Brown University who led the known as the Oort Cloud, far oxygen. But when carbon dioxide work. beyond the orbit of Neptune. If a careens into the foil at high speed, comet’s orbit brings it close to the the gold surface emits molecular “Understanding how important explosive sun, heat begins pushing cometary oxygen. ”This meant that both volcanism was on early Mars is ultimately ice off into space. This reaction atoms of oxygen come from important for understand the water produces long tails that can stretch the same CO2 [carbon dioxide] budget in Martian magma, groundwater for thousands of miles. molecule, effectively splitting it in abundance and the thickness of the an extraordinary manner,” Caltech atmosphere.” Volcanic explosions happen A team of researchers from the representatives said in a statement. when gases like water vapor are dissolved California Institute of Technology in underground magma. (Caltech) in Pasadena found a To better understand how new way to explain how comets carbon dioxide can break down When the pressure of that dissolved gas generate molecular oxygen, the into molecular oxygen, Caltech is more than the rock above can hold, it two atoms of oxygen that come chemistry professor Tom Miller and explodes, sending a fiery cloud of ash and together to form breathable air. One postdoctoral fellow Philip Shushkov lava into the air. Scientists think that these already-known method is through created a computer simulation. One kinds of eruptions should have happened kinetic energy. A sublimating challenge in modeling the reaction very early in Martian history, when there comet is a busy environment, is that the reacting molecules are was more water available to get mixed where the solar wind (the constant very “excited,” meaning they vibrate with magma. As the planet dried out, stream of particles emanating from and rotate in a complex way, the the volcanic explosions would have died the sun) can push floating water researchers said.
Recommended publications
  • The New Generation Planetary Population Synthesis (NGPPS). II
    Astronomy & Astrophysics manuscript no. pop c ESO 2020 July 14, 2020 The New Generation Planetary Population Synthesis (NGPPS) II. Planetary population of solar-like stars and overview of statistical results? Alexandre Emsenhuber1; 2, Christoph Mordasini2, Remo Burn2, Yann Alibert2, Willy Benz2, and Erik Asphaug1 1 Lunar and Planetary Laboratory, University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721, USA e-mail: [email protected] 2 Physikalisches Institut, Universität Bern, Gesselschaftsstrasse 6, 3012 Bern, Switzerland Received DD MMM YYYY / Accepted DD MMM YYYY ABSTRACT Context. Planetary formation and evolution is a combination of multiple processes that are interlinked. These processes are not known in detail and many uncertainties remain. Constraining the formation and evolution mechanisms observationally requires statistical comparison to a large diversity of planetary systems. Aims. We want to understand the global observable consequences of different physical processes (accretion, migration, and interac- tions) and initial properties (such as disc masses and metallicities) on the demographics of the planetary population. We also want to study the convergence of our scheme with respect to one initial condition, the initial number of planetary embryo in each disc. Methods. We select distributions of initial conditions that are representative of known protoplanetary discs. Then, we use the Gener- ation III Bern model to perform planetary population synthesis. We synthesise five populations with each a different initial number of Moon-mass embryos per disc: 1, 10, 20, 50, and 100. The last is our nominal planetary population consisting of 1000 stars (systems) that we use to provide an extensive statistical analysis of the planetary systems around 1 M stars.
    [Show full text]
  • Space News Update – May 2019
    Space News Update – May 2019 By Pat Williams IN THIS EDITION: • India aims to be 1st country to land rover on Moon's south pole. • Jeff Bezos says Blue Origin will land humans on moon by 2024. • China's Chang'e-4 probe resumes work for sixth lunar day. • NASA awards Artemis contract for lunar gateway power. • From airport to spaceport as UK targets horizontal spaceflight. • Russian space sector plagued by astronomical corruption. • Links to other space and astronomy news published in May 2019. Disclaimer - I claim no authorship for the printed material; except where noted (PW). INDIA AIMS TO BE 1ST COUNTRY TO LAND ROVER ON MOON'S SOUTH POLE India will become the first country to land a rover on the Moon's the south pole if the country's space agency "Indian Space Research Organisation (ISRO)" successfully achieves the feat during the country's second Moon mission "Chandrayaan-2" later this year. "This is a place where nobody has gone. All the ISRO missions till now to the Moon have landed near the Moon's equator. Chandrayaan-2, India’s second lunar mission, has three modules namely Orbiter, Lander (Vikram) & Rover (Pragyan). The Orbiter and Lander modules will be interfaced mechanically and stacked together as an integrated module and accommodated inside the GSLV MK-III launch vehicle. The Rover is housed inside the Lander. After launch into earth bound orbit by GSLV MK-III, the integrated module will reach Moon orbit using Orbiter propulsion module. Subsequently, Lander will separate from the Orbiter and soft land at the predetermined site close to lunar South Pole.
    [Show full text]
  • Determining the True Mass of Radial-Velocity Exoplanets with Gaia F
    Determining the true mass of radial-velocity exoplanets with Gaia F. Kiefer, G. Hébrard, A. Lecavelier Des Etangs, E. Martioli, S. Dalal, A. Vidal-Madjar To cite this version: F. Kiefer, G. Hébrard, A. Lecavelier Des Etangs, E. Martioli, S. Dalal, et al.. Determining the true mass of radial-velocity exoplanets with Gaia: Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. Astronomy and Astrophysics - A&A, EDP Sciences, 2021, 645, pp.A7. 10.1051/0004-6361/202039168. hal-03085694 HAL Id: hal-03085694 https://hal.archives-ouvertes.fr/hal-03085694 Submitted on 21 Dec 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A&A 645, A7 (2021) Astronomy https://doi.org/10.1051/0004-6361/202039168 & © F. Kiefer et al. 2020 Astrophysics Determining the true mass of radial-velocity exoplanets with Gaia Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets? F. Kiefer1,2, G. Hébrard1,3, A. Lecavelier des Etangs1, E. Martioli1,4, S. Dalal1, and A. Vidal-Madjar1 1 Institut d’Astrophysique de Paris, Sorbonne
    [Show full text]
  • Exoplanet Demographics Conference November 9-13, 2020 Tuesday Talk Abstracts
    Exoplanet Demographics Conference November 9-13, 2020 Tuesday Talk Abstracts Small Planets Low-mass Exoplanet Demographics - Daniel Jontof-Hutter (Univ. of the Pacific) Exoplanet science is advancing rapidly on many fronts following the detection of thousands of planets, particularly from transit surveys. Precise stellar characterization has revealed the bimodal planetary size distribution, and has enabled precise planetary mass measurements with radial velocities and transit timing. Over 120 exoplanets less massive than 30 Earths have measured masses and radii (Jontof-Hutter, 2019, AREPS, 47, 141), and a remarkably diverse range of bulk densities among these exoplanets has been revealed. Planetary mass and radius characterization has also entered the terrestrial regime- over 30 exoplanets smaller than 1.6 Earth-radii have detected masses, and planets as small as Mars now populate the mass-radius diagram. In this review, we summarize the progress that has been made in characterizing this diverse population: where planet sizes and incident fluxes inform on bulk planet properties, where compositions by volume are dominated by volatiles and where bulk planet properties within individuals systems differ substantially. To some extent, however, detection biases prevent individual characterizations from revealing underlying planet demographics. We review progress to correct for these biases in determining distributions of planet properties. Looking forward, planetary system demographics will require observations to probe system architectures beyond the compact configurations that have been detected close to stellar hosts. A small number of compact multi-transiting systems show evidence of additional planets from radial velocities, and observing campaigns to detect non-transiting planets that orbit beyond the known planets have begun.
    [Show full text]
  • School of Physics and Astronomy – Yearbook 2020
    Credit: SohebCredit: Mandhai, Physics PhD Student * SCHOOL OF PHYSICS AND ASTRONOMY – YEARBOOK 2020 Introduction Table of Contents research, and some have wandered the socially-distanced corridors with a heavy heart, missing the noise, chaos, and Introduction ....................................................... 2 energy of previous years. Many living within the city School Events & Activities ................................... 4 boundaries have been under some sort of restrictions ever since. Each of us has had to adapt, to try to find our own paths Science News .................................................... 20 through the COVID-19 pandemic, and to hold onto the certainty that better times are in front of us. From the Archive .............................................. 34 But despite the Earth-shattering events of the past year, Space Park Leicester News ................................ 37 compiling this 2020 yearbook has been remarkable, eye- Physicists Away from the Department (Socially opening, and inspiring. In the pages that follow, we hope that Distanced Edition*) .......................................... 44 you’ll be proud of the flexibility and resilience shown in the Physics and Astronomy community – the pages are Celebrating Success .......................................... 48 overflowing with School events; stories of successes in our student, research, and academic communities; highlights Meeting Members of the School ....................... 51 from our public engagement across the UK; momentous changes in our teaching through the Ignite programme; and Physics Special Topics: Editors Pick ................... 68 new leaps forward for our world-leading research. Our Comings and Goings ......................................... 70 Directors of Teaching have done a phenomenal job, working non-stop to support teaching staff who have worked tirelessly Twelve months ago, as the Leicester Physics News Team were to prepare blended courses suitable for the virtual world.
    [Show full text]
  • The Discovery of WASP-151B, WASP-153B, WASP-156B: Insights on Giant Planet Migration and the Upper Boundary of the Neptunian Desert', Astronomy and Astrophysics, Vol
    University of Birmingham The discovery of WASP-151b, WASP-153b, WASP- 156b Demangeon, Olivier D. S.; Faedi, F.; Hébrard, G.; Brown, D. J. A.; Barros, S. C. C.; Doyle, A. P.; Maxted, P. F. L.; Cameron, A. Collier; Hay, K. L.; Alikakos, J.; Anderson, D. R.; Armstrong, D. J.; Boumis, P.; Bonomo, A. S.; Bouchy, F.; Haswell, C. A.; Hellier, C.; Kiefer, F.; Lam, K. W. F.; Mancini, L. DOI: 10.1051/0004-6361/201731735 License: None: All rights reserved Document Version Publisher's PDF, also known as Version of record Citation for published version (Harvard): Demangeon, ODS, Faedi, F, Hébrard, G, Brown, DJA, Barros, SCC, Doyle, AP, Maxted, PFL, Cameron, AC, Hay, KL, Alikakos, J, Anderson, DR, Armstrong, DJ, Boumis, P, Bonomo, AS, Bouchy, F, Haswell, CA, Hellier, C, Kiefer, F, Lam, KWF, Mancini, L, McCormac, J, Norton, AJ, Osborn, HP, Palle, E, Pepe, F, Pollacco, DL, Prieto-Arranz, J, Queloz, D, Ségransan, D, Smalley, B, Triaud, AHMJ, Udry, S, West, R & Wheatley, PJ 2018, 'The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert', Astronomy and Astrophysics, vol. 610, A63. https://doi.org/10.1051/0004- 6361/201731735 Link to publication on Research at Birmingham portal Publisher Rights Statement: Checked for eligibility: 12/07/2019 This document appears in its final form in [JournalTitle], copyright © ESO 2018. The final Version of Record can be found at: https://doi.org/10.1051/0004-6361/201731735 General rights Unless a licence is specified above, all rights (including copyright and moral rights) in this document are retained by the authors and/or the copyright holders.
    [Show full text]
  • Determining the True Mass of Radial-Velocity Exoplanets with Gaia 9 Planet Candidates in the Brown-Dwarf/Stellar Regime and 27 Confirmed Planets
    Astronomy & Astrophysics manuscript no. exoplanet_mass_gaia c ESO 2020 September 30, 2020 Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets F. Kiefer1; 2, G. Hébrard1; 3, A. Lecavelier des Etangs1, E. Martioli1; 4, S. Dalal1, and A. Vidal-Madjar1 1 Institut d’Astrophysique de Paris, Sorbonne Université, CNRS, UMR 7095, 98 bis bd Arago, 75014 Paris, France 2 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France? 3 Observatoire de Haute-Provence, CNRS, Universiteé d’Aix-Marseille, 04870 Saint-Michel-l’Observatoire, France 4 Laboratório Nacional de Astrofísica, Rua Estados Unidos 154, 37504-364, Itajubá - MG, Brazil Submitted on 2020/08/20 ; Accepted for publication on 2020/09/24 ABSTRACT Mass is one of the most important parameters for determining the true nature of an astronomical object. Yet, many published exoplan- ets lack a measurement of their true mass, in particular those detected thanks to radial velocity (RV) variations of their host star. For those, only the minimum mass, or m sin i, is known, owing to the insensitivity of RVs to the inclination of the detected orbit compared to the plane-of-the-sky. The mass that is given in database is generally that of an assumed edge-on system (∼90◦), but many other inclinations are possible, even extreme values closer to 0◦ (face-on). In such case, the mass of the published object could be strongly underestimated by up to two orders of magnitude.
    [Show full text]
  • Possible Atmospheric Diversity of Low Mass Exoplanets – Some Central Aspects J.L
    Possible Atmospheric Diversity of Low Mass Exoplanets – Some Central Aspects J.L. Grenfell, J. Leconte, F. Forget, M. Godolt, O. Carrión-González, L. Noack, F. Tian, H. Rauer, Fabrice Gaillard, E. Bolmont, et al. To cite this version: J.L. Grenfell, J. Leconte, F. Forget, M. Godolt, O. Carrión-González, et al.. Possible Atmospheric Diversity of Low Mass Exoplanets – Some Central Aspects. Space Science Reviews, Springer Verlag, 2020, 216 (5), 10.1007/s11214-020-00716-4. insu-02917578 HAL Id: insu-02917578 https://hal-insu.archives-ouvertes.fr/insu-02917578 Submitted on 5 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 1 Possible Atmospheric Diversity of Low Mass Exoplanets – some Central Aspects 2 3 John Lee Grenfell1, Jeremy Leconte2, François Forget3, Mareike Godolt4,Óscar Carrión-González4, Lena Noack5, 4 Feng Tian6, Heike Rauer1,4,5, Fabrice Gaillard7, Émeline Bolmont8, Benjamin Charnay9 and Martin Turbet8 5 6 (1) Institut für Planetenforschung (PF) 7 Deutsches Zentrum für Luft- und Raumfahrt (DLR) 8 Rutherfordstr. 2 9 12489 Berlin 10 Germany 11 12 (2) Laboratoire d’Astrophysique de Bordeaux (LAB) 13 Université Bordeaux 14 Centre National de la Recherche Scientifique (CNRS) B18N 15 Alle Geoffroy Saint-Hilaire 16 33615 Pessac 17 France 18 19 (3) Laboratoire de Météorologie Dynamique (LMD) 20 Institut Pierre Simon Laplace Université 21 4 Place Jussieu 22 75005 Paris 23 France 24 25 (4) Zentrum für Astronomie und Astrophysik (ZAA) 26 Technische Universität Berlin (TUB) 27 Hardenbergstr.
    [Show full text]
  • A Remnant Planetary Core in the Hot Neptunian Desert
    A remnant planetary core in the hot Neptunian desert Armstrong, D. J., Lopez, T. A., Adibekyan, V., Booth, R. A., Bryant, E. M., Collins, K. A., Emsenhuber, A., Huang, C. X., King, G. W., Lillo-box, J., Lissauer, J. J., Matthews, E. C., Mousis, O., Nielsen, L. D., Osborn, H., Otegi, J., Santos, N. C., Sousa, S. G., Stassun, K. G., ... Zhan, Z. (2020). A remnant planetary core in the hot Neptunian desert. Nature, 583(2020), 32. https://doi.org/10.1038/s41586-020-2421-7 Published in: Nature Document Version: Peer reviewed version Queen's University Belfast - Research Portal: Link to publication record in Queen's University Belfast Research Portal Publisher rights Copyright 2020 Nature. This work is made available online in accordance with the publisher’s policies. Please refer to any applicable terms of use of the publisher. General rights Copyright for the publications made accessible via the Queen's University Belfast Research Portal is retained by the author(s) and / or other copyright owners and it is a condition of accessing these publications that users recognise and abide by the legal requirements associated with these rights. Take down policy The Research Portal is Queen's institutional repository that provides access to Queen's research output. Every effort has been made to ensure that content in the Research Portal does not infringe any person's rights, or applicable UK laws. If you discover content in the Research Portal that you believe breaches copyright or violates any law, please contact [email protected]. Download date:24. Sep. 2021 Draft version March 24, 2020 Typeset using LATEX default style in AASTeX62 A remnant planetary core in the hot Neptunian desert David J.
    [Show full text]
  • Summary of Ground Based Surveys
    Summary of ground based (transit) surveys Don Pollacco University of Warwick History: First Detec.ons 2 Outline Why transits are important? Limitations of the technique 20 years since the first exoplanet transit - Results from historical surveys - First generation - Second generation Current/future surveys – what are they doing? – synergy with TESS Why transit detections are so important Accurate and (mostly) physics independent measurement of planetary radius - Main limita8on is our understanding of the physical proper8es of stars Accurate and (mostly) physics independent measurement of orbital inclina8on - Main limita8on is our understanding of limb darkening Scien8fically - Atmospheres, bulk planetary parameters, RM etc Transit survey limitations Very inefficient – geometric probability low eg 4d -> ~10% probability Mimics – addi>onal observa>ons needed to rule out Stellar ac>vity Ac>vity a problem for detec>on but more serious for RV spectroscopy The scene in 2001….. Horne 2003 6 Correlated noise White Red White + Red Where Cij is the covariance coefficients between the ith and Pont, Zucker, Queloz 2006 jth measurements (during the transit) 7 First Generation Surveys HAT (62), Multi-site (longitude) 7 instruments TRES (5), WASP (192), 1 faCility in eaCh hemisphere XO (7) HAT/WASP/XO all used large aperture short foCus camera lenses = > lots of systematics Ground based transits: SuperWASP SW-N La Palma SW-N La Palma SW-S SAAO SW discovery 2m LT WASP project is the leading survey with >190 confirmed planets. Largest, lowest density, backward orbit, highest irradiaDon etc Second Generation Surveys Surveys designed to look at low luminosity stars (red dwarfs) MEarth M0-5 (3) North and South Apache M0-5 (0) Qatar K (10) Mearth - Monitoring individual M dwarfs Quality not quantity….
    [Show full text]
  • Downloaded At
    Manuscript version: Author’s Accepted Manuscript The version presented in WRAP is the author’s accepted manuscript and may differ from the published version or Version of Record. Persistent WRAP URL: http://wrap.warwick.ac.uk/134820 How to cite: Please refer to published version for the most recent bibliographic citation information. If a published version is known of, the repository item page linked to above, will contain details on accessing it. Copyright and reuse: The Warwick Research Archive Portal (WRAP) makes this work by researchers of the University of Warwick available open access under the following conditions. Copyright © and all moral rights to the version of the paper presented here belong to the individual author(s) and/or other copyright owners. To the extent reasonable and practicable the material made available in WRAP has been checked for eligibility before being made available. Copies of full items can be used for personal research or study, educational, or not-for-profit purposes without prior permission or charge. Provided that the authors, title and full bibliographic details are credited, a hyperlink and/or URL is given for the original metadata page and the content is not changed in any way. Publisher’s statement: Please refer to the repository item page, publisher’s statement section, for further information. For more information, please contact the WRAP Team at: [email protected]. warwick.ac.uk/lib-publications Draft version March 16, 2020 Typeset using LATEX manuscript style in AASTeX62 A remnant planetary core in the hot Neptunian desert 1, 2, ∗ 3 4 5 1 David J.
    [Show full text]
  • Planets Solar System Paper Contents
    Planets Solar system paper Contents 1 Jupiter 1 1.1 Structure ............................................... 1 1.1.1 Composition ......................................... 1 1.1.2 Mass and size ......................................... 2 1.1.3 Internal structure ....................................... 2 1.2 Atmosphere .............................................. 3 1.2.1 Cloud layers ......................................... 3 1.2.2 Great Red Spot and other vortices .............................. 4 1.3 Planetary rings ............................................ 4 1.4 Magnetosphere ............................................ 5 1.5 Orbit and rotation ........................................... 5 1.6 Observation .............................................. 6 1.7 Research and exploration ....................................... 6 1.7.1 Pre-telescopic research .................................... 6 1.7.2 Ground-based telescope research ............................... 7 1.7.3 Radiotelescope research ................................... 8 1.7.4 Exploration with space probes ................................ 8 1.8 Moons ................................................. 9 1.8.1 Galilean moons ........................................ 10 1.8.2 Classification of moons .................................... 10 1.9 Interaction with the Solar System ................................... 10 1.9.1 Impacts ............................................ 11 1.10 Possibility of life ........................................... 12 1.11 Mythology .............................................
    [Show full text]