Conferences related to Extrasolar planetary mass

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2020 IEEE International Conference on Plasma Science (ICOPS)

IEEE International Conference on Plasma Science (ICOPS) is an annual conference coordinated by the Plasma Science and Application Committee (PSAC) of the IEEE Nuclear & Plasma Sciences Society.


2019 Conference on Lasers and Electro-Optics Europe & European Quantum Electronics Conference (CLEO/Europe-EQEC)

CLEO®/Europe will showcase the latest developments in a wide range of laser and photonics areas including laser source development, materials, ultrafast science, fibre optics, nonlinear optics, terahertz sources, high-field physics, optical telecommunications, nanophotonics, biophotonics.EQEC will feature the fundamentals of quantum optics, quantum information, atom optics, ultrafast optics, nonlinear phenomena and self-organization, plasmonics and metamaterials, fundamental nanooptics, theoretical and computational photonics.


2019 IEEE Aerospace Conference

The international IEEE Aerospace Conference is organized to promote interdisciplinaryunderstanding of aerospace systems, their underlying science, and technology



Periodicals related to Extrasolar planetary mass

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Spectrum, IEEE

IEEE Spectrum Magazine, the flagship publication of the IEEE, explores the development, applications and implications of new technologies. It anticipates trends in engineering, science, and technology, and provides a forum for understanding, discussion and leadership in these areas. IEEE Spectrum is the world's leading engineering and scientific magazine. Read by over 300,000 engineers worldwide, Spectrum provides international coverage of all ...



Most published Xplore authors for Extrasolar planetary mass

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Xplore Articles related to Extrasolar planetary mass

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Detecting exoplanets with extreme adaptive optics and a single-mode fibre fed spectrograph

2013 Conference on Lasers & Electro-Optics Europe & International Quantum Electronics Conference CLEO EUROPE/IQEC, 2013

A key technique used to detect and characterise exoplanets is Doppler spectroscopy. The technique involves measuring the amplitude of the periodic wavelength shift in the absorption lines of a star due to the physical wobble in the star brought on by the presence of an unseen orbiting planetary-mass companion. From the periodicity and the magnitude of the wobble velocity, it ...


In search of alien worlds

IEEE Spectrum, 2012

In order to hunt a key component for planets like our own, astronomer Francesco Pepe will use the fiber to feed star light into a new detector-the High Accuracy Radial velocity Planet Searcher-North (HARPS-N), an ultraprecise spectrograph that is being assembled nearby, not far from a field of grazing horses. In the coming months, Pepe, an astronomer, and his colleagues ...



Educational Resources on Extrasolar planetary mass

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IEEE.tv Videos

ITEC 2014: Urban Mass Transit Systems: Current Status and Future Trends
Virtual World Symposium - Moon World
Robotics History: Narratives and Networks Oral Histories:Brian Wilcox
Inspiring Brilliance: The Impact on Astronomy of Maxwell's Adams' Prize Essay
Intelligent Systems for Deep Space Exploration: Solutions and Challenges - Roberto Furfaro
From Automatic People Movers to Fully Automated Mass Transit Systems
IROS TV 2019- How to Build a Robot: Vision Based Estimation of Driving Energy for Planetary Rovers
IROS TV 2019- Macau- Episode 2- Robots Connecting People
Technologies for Terahertz Science
Injury Evaluation of Human-Robot Impacts
Transportation Electrification: Green Public & Comercial Transportation
New Results from the G2 Axion Dark Matter Experiment - Applied Superconductivity Conference 2018
Breaking Spectral and Performance Barriers for Diode Lasers - Plenary Speaker, Manijeh Razeghi - IPC 2018
Expert Panel: Opportunity Landscape Review - Internet Inclusion: Global Connect Stakeholders Advancing Solutions, Washington DC, 2016
IROS TV 2019-STAR LAB at the University of Surrey Space Technology for Autonomous systems & Robotics
Soft Robotics & Biologically Inspired Robotics at Carnegie Mellon University
Superconducting Detectors for Astrophysics and Cosmology - ASC-2014 Plenary series - 9 of 13 - Thursday 2014/8/14
Quadrotor Trajectory Tracking with L1 Optimal control
Q&A with Mark Papermaster: IEEE Rebooting Computing Podcast, Episode 15
Q&A with Dr. Bill Tonti: IEEE Rebooting Computing Podcast, Episode 3

IEEE-USA E-Books

  • Detecting exoplanets with extreme adaptive optics and a single-mode fibre fed spectrograph

    A key technique used to detect and characterise exoplanets is Doppler spectroscopy. The technique involves measuring the amplitude of the periodic wavelength shift in the absorption lines of a star due to the physical wobble in the star brought on by the presence of an unseen orbiting planetary-mass companion. From the periodicity and the magnitude of the wobble velocity, it is possible to constrain parameters about the exoplanet such as mass, distance from the star, period and so on. This information is necessary for determining if the planet is likely to have the correct chemical composition in order to support life and if it is within the habitable zone (the region around a star where it is possible to support water in the liquid phase).

  • In search of alien worlds

    In order to hunt a key component for planets like our own, astronomer Francesco Pepe will use the fiber to feed star light into a new detector-the High Accuracy Radial velocity Planet Searcher-North (HARPS-N), an ultraprecise spectrograph that is being assembled nearby, not far from a field of grazing horses. In the coming months, Pepe, an astronomer, and his colleagues will take apart the go-cart-size instrument, box up the pieces, and put them together again in a room near Italy's Telescopio Nazionale Galileo on La Palma, one of the Canary Islands. When HARPS-N begins observations in April, astronomers expect it will be the most precise planet hunter in the northern hemisphere. They also reckon it will be particularly well placed to help bag the most coveted extrasolar quarry of all-planets small enough to have rocky surfaces and cool enough to have liquid water.



Standards related to Extrasolar planetary mass

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No standards are currently tagged "Extrasolar planetary mass"


Jobs related to Extrasolar planetary mass

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