Grant: Discovery Grants Program - Individual
York University
$52,000.00
Diversity of the Sub-Stellar Realm
FY 2015-16
Summary
After millennia of speculation and a century of false starts, astronomers have found hundreds of confirmed planets and thousands more planet candidates around other stars since the mid-1990s. The pace of discovery continues to accelerate, as different (and often complementary) detection techniques mature, and as more capable ground- and space-based instruments come into play. Meanwhile, the past two decades have also witnessed the identification of a new class of astronomical objects called ""brown dwarfs"", which straddle the boundary between stars and planets. The two types of objects -planets and brown dwarfs- are collectively referred to as sub-stellar objects. I propose an ambitious, multi-faceted research program, using state-of-the-art instruments on several of the world's largest telescopes, to investigate the diversity of sub-stellar objects. Specifically, I propose to (1) characterize close-in transiting planets using data from the Kepler space telescope as well as innovative high-precision observations with ground-based telescopes; (2) search for and characterize sub-stellar companions of nearby young stars through high-contrast, high-angular-resolution imaging and spectroscopy; and (3) identify and characterize the lowest mass isolated brown dwarfs using deep wide-field surveys of nearby young star clusters and follow-up spectroscopy. The proposed work will not only advance our understanding of the origins, evolution and diversity of planets and brown dwarfs, but also contribute to the emerging research area of `comparative exoplanetology'.
Program
Discovery Grants Program - Individual
Recipient
Location
Ontario, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
312092-2013
Name nom
Jayawardhana, Ray
Department département
Science, Faculty of
Organization id
38
Institution établissement
York University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2015
Competition year année de concours
2013
Award amount
52000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
Area of application code
1204
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Space and astronomy
Area of application fr
Sciences spatiales et astronomie
Research subject code
3203
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Galactic
Research subject fr
Galactique
Partie
3
Nb partie
5
Application title
Diversity of the Sub-Stellar Realm
Keyword
NSERC
Application summary
After millennia of speculation and a century of false starts, astronomers have found hundreds of confirmed planets and thousands more planet candidates around other stars since the mid-1990s. The pace of discovery continues to accelerate, as different (and often complementary) detection techniques mature, and as more capable ground- and space-based instruments come into play. Meanwhile, the past two decades have also witnessed the identification of a new class of astronomical objects called ""brown dwarfs"", which straddle the boundary between stars and planets. The two types of objects -planets and brown dwarfs- are collectively referred to as sub-stellar objects. I propose an ambitious, multi-faceted research program, using state-of-the-art instruments on several of the world's largest telescopes, to investigate the diversity of sub-stellar objects. Specifically, I propose to (1) characterize close-in transiting planets using data from the Kepler space telescope as well as innovative high-precision observations with ground-based telescopes; (2) search for and characterize sub-stellar companions of nearby young stars through high-contrast, high-angular-resolution imaging and spectroscopy; and (3) identify and characterize the lowest mass isolated brown dwarfs using deep wide-field surveys of nearby young star clusters and follow-up spectroscopy. The proposed work will not only advance our understanding of the origins, evolution and diversity of planets and brown dwarfs, but also contribute to the emerging research area of `comparative exoplanetology'.