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Michael Garcia Hubble Space Telescope Users Committee (STUC)
Hubble Space Telescope Users Committee (STUC) April 16, 2015 Michael Garcia HST Program Scientist [email protected] 1 Hubble Sees Supernova Split into Four Images by Cosmic Lens 2 NASA’s Hubble Observations suggest Underground Ocean on Jupiter’s Largest Moon Ganymede file:///Users/ file:///Users/ mrgarci2/Desktop/mrgarci2/Desktop/ hs-2015-09-a-hs-2015-09-a- web.jpg web.jpg 3 NASA’s Hubble detects Distortion of Circumstellar Disk by a Planet 4 The Exoplanet Travel Bureau 5 TESS Transiting Exoplanet Survey Satellite CURRENT STATUS: • Downselected April 2013. • Major partners: - PI and science lead: MIT - Project management: NASA GSFC - Instrument: Lincoln Laboratory - Spacecraft: Orbital Science Corp • Agency launch readiness date NLT June 2018 (working launch date August 2017). • High-Earth elliptical orbit (17 x 58.7 Earth radii). Standard Explorer (EX) Mission PI: G. Ricker (MIT) • Development progressing on plan. Mission: All-Sky photometric exoplanet - Systems Requirement Review (SRR) mapping mission. successfully completed on February Science goal: Search for transiting 12-13, 2014. exoplanets around the nearby, bright stars. Instruments: Four wide field of view (24x24 - Preliminary Design Review (PDR) degrees) CCD cameras with overlapping successfully completed Sept 9-12, 2014. field of view operating in the Visible-IR - Confirmation Review, for approval to enter spectrum (0.6-1 micron). implementation phase, successfully Operations: 3-year science mission after completed October 31, 2014. launch. - Mission CDR on track for August 2015 6 JWST Hardware Progress JWST remains on track for an October 2018 launch within its replan budget guidelines 7 WFIRST / AFTA Widefield Infrared Survey Telescope with Astrophysics Focused Telescope Assets Coronagraph Technology Milestones Widefield Detector Technology Milestones 1 Shaped Pupil mask fabricated with reflectivity of 7/21/14 1 Produce, test, and analyze 2 candidate 7/31/14 -4 10 and 20 µm pixel size. -
Linking Stars, Planets and Debris Through Herschel Observations of Radial Velocity Exoplanet Host Stars
Linking stars, planets and debris through Herschel observations of radial velocity exoplanet host stars Jonathan P. Marshall Universidad Autónoma de Madrid Introduction • Herschel observed 104 radial velocity exoplanet host stars, of which 30 also had detectable circumstellar discs (DEBRIS, DUNES, GT and SKARPS) • Given that we expect planets to form from the agglomeration of planetesimals, there should be some link between the two • Previous work with Spitzer identified no correlation between planets and debris (Moro-martin et al. 2007, Bryden et al. 2009) • Observational signatures of planets may be visible in the spatial distribution of dust discs around other stars Imaging exoplanets • We find exoplanets in systems with debris discs (Marois et al. 2008; Bonnefoy et al. 2011; Rameau et al. 2013) Multi-component discs • HIP 17439’s debris disc is potentially the result of two cold dust belts Ertel et al. 2014 Schueppler et al., subm. Dynamical interactions • e.g. Eta Corvi’s Spitzer IRS spectrum shows evidence for KBO material in inner system Matthews et al. 2010 Lisse et al. 2012 Perturbation • Stars hosting exoplanets with low orbital eccentricities show a weak tendency to have brighter discs • Planets with lower eorb are less disruptive to parent bodies in debris belts Maldonado et al. 2012 Eccentric discs • e.g. HIP 15371 • Asymmetric structure proposed to be the result of dynamical perturbation by a planetary companion . Similar evidence seen in other discs (in sub-mm) tends to be weak, potentially result of low s/n observation . Not necessarily a planet, as remnant gas could affect dust Faramaz et al. 2014 Coplanarity • Inclination of star, i*, and disc, id • Debris discs are generally seen to lie along the equatorial plane of the host star • Few exceptions, e.g. -
Protoplanetary Disks and Debris Disks
Protoplanetary Disks and Debris Disks David J. Wilner Harvard-Smithsonian Center for Astrophysics Sean Andrews Meredith Hughes Chunhua Qi June 12, 2009 Millimeter and Submillimeter Astronomy, Taipei Image: NASA/JPL-Caltech/T. Pyle (SSC) Circumstellar Disks • inevitable consequence of gravity + angular momentum • integral part of star and planet formation paradigm 4 10 yr 105 yr 7 10 yr 108 yr 100 AU cloud collapse protostar protoplanetary disk planetary system and debris disk Marrois et al. 2008 J. Jørgensen Isella et al. 2007 Alves et al. 2001 2 This Talk • context: “protoplanetary” and “debris” disks • tool: submillimeter dust continuum emission • some recent SMA studies and implications 1. high resolution ρ Oph disk imaging survey - S. Andrews, D. Wilner, A.M. Hughes, C. Qi, K. Dullemond (arxiv:0906.0730) 2. resolved disk polarimetry: TW Hya, HD 163296 - A.M. Hughes, D. Wilner, J. Cho, D. Marrone, A. Lazarian, S. Andrews, R. Rao 3. debris disk imaging: HD 107146 - D. Wilner, J. Williams, S. Andrews, A.M. Hughes, C. Qi 3 “Protoplanetary” → “Debris” McCaughrean et al. 1995; Burrows et al. 1996 Corder et al 2009; Greaves et al. 2005 V. Pietu; Isella et al. 2007 Kalas et al. 2008; Marois et al. 2008 • age ~1 to 10 Myr • age up to Gyrs • gas and trace dust • dust and trace gas • dust particles are sticking, • planetesimals are colliding, growing into planetesimals creating new dust particles • mass 0.001 to 0.1 M • mass <1 Mmoon • mass distribution? • dust distribution → planets? • accretion/dispersal physics? • dynamical history? 4 Submillimeter Dust Emission x-ray uv optical infrared submm cm hot gas/accr. -
RADIAL VELOCITIES in the ZODIACAL DUST CLOUD
A SURVEY OF RADIAL VELOCITIES in the ZODIACAL DUST CLOUD Brian Harold May Astrophysics Group Department of Physics Imperial College London Thesis submitted for the Degree of Doctor of Philosophy to Imperial College of Science, Technology and Medicine London · 2007 · 2 Abstract This thesis documents the building of a pressure-scanned Fabry-Perot Spectrometer, equipped with a photomultiplier and pulse-counting electronics, and its deployment at the Observatorio del Teide at Izaña in Tenerife, at an altitude of 7,700 feet (2567 m), for the purpose of recording high-resolution spectra of the Zodiacal Light. The aim was to achieve the first systematic mapping of the MgI absorption line in the Night Sky, as a function of position in heliocentric coordinates, covering especially the plane of the ecliptic, for a wide variety of elongations from the Sun. More than 250 scans of both morning and evening Zodiacal Light were obtained, in two observing periods – September-October 1971, and April 1972. The scans, as expected, showed profiles modified by components variously Doppler-shifted with respect to the unshifted shape seen in daylight. Unexpectedly, MgI emission was also discovered. These observations covered for the first time a span of elongations from 25º East, through 180º (the Gegenschein), to 27º West, and recorded average shifts of up to six tenths of an angstrom, corresponding to a maximum radial velocity relative to the Earth of about 40 km/s. The set of spectra obtained is in this thesis compared with predictions made from a number of different models of a dust cloud, assuming various distributions of dust density as a function of position and particle size, and differing assumptions about their speed and direction. -
Astro2020 Science White Paper Modeling Debris Disk Evolution
Astro2020 Science White Paper Modeling Debris Disk Evolution Thematic Areas Planetary Systems Formation and Evolution of Compact Objects Star and Planet Formation Cosmology and Fundamental Physics Galaxy Evolution Resolved Stellar Populations and their Environments Stars and Stellar Evolution Multi-Messenger Astronomy and Astrophysics Principal Author András Gáspár Steward Observatory, The University of Arizona [email protected] 1-(520)-621-1797 Co-Authors Dániel Apai, Jean-Charles Augereau, Nicholas P. Ballering, Charles A. Beichman, Anthony Boc- caletti, Mark Booth, Brendan P. Bowler, Geoffrey Bryden, Christine H. Chen, Thayne Currie, William C. Danchi, John Debes, Denis Defrère, Steve Ertel, Alan P. Jackson, Paul G. Kalas, Grant M. Kennedy, Matthew A. Kenworthy, Jinyoung Serena Kim, Florian Kirchschlager, Quentin Kral, Sebastiaan Krijt, Alexander V. Krivov, Marc J. Kuchner, Jarron M. Leisenring, Torsten Löhne, Wladimir Lyra, Meredith A. MacGregor, Luca Matrà, Dimitri Mawet, Bertrand Mennes- son, Tiffany Meshkat, Amaya Moro-Martín, Erika R. Nesvold, George H. Rieke, Aki Roberge, Glenn Schneider, Andrew Shannon, Christopher C. Stark, Kate Y. L. Su, Philippe Thébault, David J. Wilner, Mark C. Wyatt, Marie Ygouf, Andrew N. Youdin Co-Signers Virginie Faramaz, Kevin Flaherty, Hannah Jang-Condell, Jérémy Lebreton, Sebastián Marino, Jonathan P. Marshall, Rafael Millan-Gabet, Peter Plavchan, Luisa M. Rebull, Jacob White Abstract Understanding the formation, evolution, diversity, and architectures of planetary systems requires detailed knowledge of all of their components. The past decade has shown a remarkable increase in the number of known exoplanets and debris disks, i.e., populations of circumstellar planetes- imals and dust roughly analogous to our solar system’s Kuiper belt, asteroid belt, and zodiacal dust. -
Exep Science Plan Appendix (SPA) (This Document)
ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 1 of 61 Created By: David A. Breda Date Program TDEM System Engineer Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Nick Siegler Date Program Chief Technologist Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology Concurred By: Dr. Gary Blackwood Date Program Manager Exoplanet Exploration Program NASA/Jet Propulsion Laboratory California Institute of Technology EXOPDr.LANET Douglas Hudgins E XPLORATION PROGRAMDate Program Scientist Exoplanet Exploration Program ScienceScience Plan Mission DirectorateAppendix NASA Headquarters Karl Stapelfeldt, Program Chief Scientist Eric Mamajek, Deputy Program Chief Scientist Exoplanet Exploration Program JPL CL#19-0790 JPL Document No: 1735632 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 2 of 61 Approved by: Dr. Gary Blackwood Date Program Manager, Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory Dr. Douglas Hudgins Date Program Scientist Exoplanet Exploration Program Science Mission Directorate NASA Headquarters Created by: Dr. Karl Stapelfeldt Chief Program Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology Dr. Eric Mamajek Deputy Program Chief Scientist Exoplanet Exploration Program Office NASA/Jet Propulsion Laboratory California Institute of Technology This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. © 2018 California Institute of Technology. Government sponsorship acknowledged. Exoplanet Exploration Program JPL CL#19-0790 ExEP Science Plan, Rev A JPL D: 1735632 Release Date: February 15, 2019 Page 3 of 61 Table of Contents 1. -
Solar System Debris Disk - S2D2
Solar System Debris Disk - S2D2 Image credit: NASA/JPL-Caltech Proposal for Science Themes of ESA's L2 and L3 Missions Ralf Srama Universität Stuttgart, Institut für Raumfahrtsysteme Raumfahrtzentrum Baden Württemberg Pfaffenwaldring 29, 70569 Stuttgart [email protected] Tel. +49 711 6856 2511, Fax +49 711 685 63596 http://www.irs.uni-stuttgart.de 2 Solar System Debris Disk - S2D2 Contributors Eberhard Grün, Max-Planck-Institut für Kernphysik, Heidelberg, Germany Alexander Krivov, Astrophysikalisches Institut, Univ. Jena, Germany Rachel Soja, Institut für Raumfahrtsysteme, Univ. Stuttgart, Germany Veerle Sterken, Institut für Raumfahrtsysteme, Univ. Stuttgart, Germany Zoltan Sternovsky, LASP, Univ. of Colorado, Boulder, USA. Supporters listed at http://www.dsi.uni-stuttgart.de/cosmicdust/missions/debrisdisk/index.html 3 Solar System Debris Disk - S2D2 Summary from direct observations of the parent bodies. The sizes of these parent bodies range from Understanding the conditions for planet Near Earth Asteroids with sizes of a few 10 m, formation is the primary theme of ESA's to km-sized comet nuclei, to over 1000 km- Cosmic Vision plan. Planets and left-over sized Trans-Neptunian Objects. The inner small solar system bodies are witnesses and zodiacal dust cloud has been probed by remote samples of the processing in different regions sensing instruments at visible and infrared of the protoplanetary disk. Small bodies fill the wavelengths, micro crater counts, in situ dust whole solar system from the surface of the analyzers, meteor observations and recent sun, to the fringes of the solar system, and to sample return missions. Nevertheless, the the neighboring stellar system. This is covered dynamical and compositional interrelations by the second theme of Cosmic Vision. -
Space Missions for Exoplanet
Space missions for exoplanet January 3, 2020 Source: The Hindu Manifest pedagogy: As a part of science & technology and geography, questions related to space have been asked both at prelims and mains stage. Finding life in other celestial bodies had always been a human curiosity. Origin of the solar system, exoplanets as prospective resources zone, finding life etc are key objectives of NASA and other space programs. In news: European Space Agency (ESA) has launched CHEOPS exoplanet mission Placing it in syllabus: Exoplanet space missions Static dimensions: What are exoplanets? Current dimensions: Exoplanet missions by NASA Exoplanet missions by ESA and CHEOPS mission Content: What are Exoplanets? The worlds orbiting other stars are called “exoplanets”. They vary in sizes, from gas giants larger than Jupiter to small, rocky planets about as big around as Earth. They can be hot enough to boil metal or locked in deep freeze. They can orbit two suns at once. Some exoplanets are sunless, wandering through the galaxy in permanent darkness. The first exoplanet invented was 51 Pegasi b, a “hot Jupiter” in 1995 which is 50 light-years away that is locked in a four-day orbit around its star. ((The discoverers Didier Queloz and Michel Mayor of 51 Pegasi b shared the 2019 Nobel Prize in Physics for their breakthrough finding)). And a system of three “pulsar planets” had been detected, beginning in 1992. The circumstellar habitable zone (CHZ) also called the Goldilocks zone is the range of orbits around a star within which a planetary surface can support liquid water given sufficient atmospheric pressure. -
Elements of Astronomy and Cosmology Outline 1
ELEMENTS OF ASTRONOMY AND COSMOLOGY OUTLINE 1. The Solar System The Four Inner Planets The Asteroid Belt The Giant Planets The Kuiper Belt 2. The Milky Way Galaxy Neighborhood of the Solar System Exoplanets Star Terminology 3. The Early Universe Twentieth Century Progress Recent Progress 4. Observation Telescopes Ground-Based Telescopes Space-Based Telescopes Exploration of Space 1 – The Solar System The Solar System - 4.6 billion years old - Planet formation lasted 100s millions years - Four rocky planets (Mercury Venus, Earth and Mars) - Four gas giants (Jupiter, Saturn, Uranus and Neptune) Figure 2-2: Schematics of the Solar System The Solar System - Asteroid belt (meteorites) - Kuiper belt (comets) Figure 2-3: Circular orbits of the planets in the solar system The Sun - Contains mostly hydrogen and helium plasma - Sustained nuclear fusion - Temperatures ~ 15 million K - Elements up to Fe form - Is some 5 billion years old - Will last another 5 billion years Figure 2-4: Photo of the sun showing highly textured plasma, dark sunspots, bright active regions, coronal mass ejections at the surface and the sun’s atmosphere. The Sun - Dynamo effect - Magnetic storms - 11-year cycle - Solar wind (energetic protons) Figure 2-5: Close up of dark spots on the sun surface Probe Sent to Observe the Sun - Distance Sun-Earth = 1 AU - 1 AU = 150 million km - Light from the Sun takes 8 minutes to reach Earth - The solar wind takes 4 days to reach Earth Figure 5-11: Space probe used to monitor the sun Venus - Brightest planet at night - 0.7 AU from the -
Exoplanetary Transits As Seen by Gaia
Highlights of Spanish Astrophysics VII, Proceedings of the X Scientific Meeting of the Spanish Astronomical Society held on July 9 - 13, 2012, in Valencia, Spain. J. C. Guirado, L.M. Lara, V. Quilis, and J. Gorgas (eds.) Exoplanetary transits as seen by Gaia H. Voss1;2, C. Jordi1;2;3, C. Fabricius1;2, J. M. Carrasco1;2, E. Masana1;2, and X. Luri1;2;3 1 IEEC: Institut d'Estudis Espacials de Catalunya 2 ICC-UB: Institut de Ci`encesdel Cosmos de la Universitat de Barcelona 3 UB: Departament d'Astronomia i Meteorologia, Universitat de Barcelona Abstract The ESA cornerstone mission Gaia will be launched in 2013 to begin a scan of about one billion sources in the Milky Way and beyond. During the mission time of 5 years (+ one year extension) repeated astrometric, photometric and spectroscopic observations of the entire sky down to magnitude 20 will be recorded. Therefore, Gaia as an All-Sky survey has enormous potential for discovery in almost all fields of astronomy and astrophysics. Thus, 50 to 200 epoch observations will be collected during the mission for about 1 billion sources. Gaia will also be a nearly unbiased survey for transiting extrasolar planets. Based on latest detection probabilities derived from the very successful NASA Kepler mis- sion, our knowledge about the expected photometric precision of Gaia in the white-light G band and the implications due to the Gaia scanning law, we have analysed how many transiting exoplanets candidates Gaia will be able to detect. We include the entire range of stellar types in the parameter space for our analysis as potential host stars, as they will be observed by Gaia. -
Telescope to Seek Dust Where Other Earths May Lie 22 January 2015, by Whitney Clavin
Telescope to seek dust where other Earths may lie 22 January 2015, by Whitney Clavin The new instrument, based at the Large Binocular Telescope Observatory at the top of Mount Graham in southeastern Arizona, will obtain the best infrared images yet of dust permeating a star's habitable zone, the region around the star where water—an essential ingredient for life as we know it—could pool on a planet. Earth sits comfortably within our sun's habitable zone, hence its glistening surface of oceans. Scientists want to take pictures of exo-Earths and break up their light into a rainbow of colors. This color information is displayed in plots, called The Large Binocular Telescope Interferometer (LBTI) spectra, which reveal chemical clues about whether instrument set its eyes on a dusty star system called Eta a planet could sustain life. But dust—which comes Corvi, depicted here in this artist's concept. Recent from colliding asteroids and evaporating collisions between comets and rocky bodies within the comets—can outshine the feeble light of a planet, star system are thought to have generated the surplus of making this task difficult. dust. Credit: Large Binocular Telescope Observatory "Imagine trying to view a firefly buzzing around a lighthouse in Canada from Los Angeles," said Denis Defrère of the University of Arizona, lead The NASA-funded Large Binocular Telescope author of the new study that appears in the Jan. 14 Interferometer, or LBTI, has completed its first issue of the Astrophysical Journal. "Now imagine study of dust in the "habitable zone" around a star, that fog is in the way. -
1 Director's Message
1 Director’s Message Markus Kissler-Patig 3 Weighing the Black Hole in M101 ULX-1 Stephen Justham and Jifeng Liu 8 World’s Most Powerful Planet Finder Turns its Eye to the Sky: First Light with the Gemini Planet Imager Bruce Macintosh and Peter Michaud 12 Science Highlights Nancy A. Levenson 15 Operations Corner: Update and 2013 Review Andy Adamson 20 Instrumentation Development: Update and 2013 Review Scot Kleinman ON THE COVER: GeminiFocus January 2014 The cover of this issue GeminiFocus is a quarterly publication of Gemini Observatory features first light images from the Gemini 670 N. A‘ohoku Place, Hilo, Hawai‘i 96720 USA Planet Imager that Phone: (808) 974-2500 Fax: (808) 974-2589 were released at the Online viewing address: January 2014 meeting www.gemini.edu/geminifocus of the American Managing Editor: Peter Michaud Astronomical Society Science Editor: Nancy A. Levenson held in Washington, D.C. Associate Editor: Stephen James O’Meara See the press release Designer: Eve Furchgott / Blue Heron Multimedia that accompanied the images starting on Any opinions, findings, and conclusions or recommendations page 8 of this issue. expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation. Markus Kissler-Patig Director’s Message 2013: A Successful Year for Gemini! As 2013 comes to an end, we can look back at 12 very successful months for Gemini despite strong budget constraints. Indeed, 2013 was the first stage of our three-year transition to a reduced opera- tions budget, and it was marked by a roughly 20 percent cut in contributions from Gemini’s partner countries.