Download Powerpoint presentation from AAS press

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts
no text concepts found
Transcript
The Smallest Planet Orbiting
the Smallest Star
David Bennett
University of Notre Dame
for the MOA & OGLE Collaborations
mobile phone: 574-315-6621
Summary of Finding
• MOA-2007-BLG-192Lb is a ~3 Earth-mass
planet
– this is the smallest discovered to date
• Its host star has a mass of 6  3% of the mass
of the Sun
– Most likely, it is < 8% of a Solar mass, which is too
small to sustain nuclear reactions - a brown dwarf
• The system is at a distance of 3000 light years
• The planet’s orbital radius is about the same as
that of Venus (70% of the Earth-Sun distance)
David Bennett - Smallest Planet Orbits Smallest Star
Host Color Is Probably Magenta
• “Brown” Dwarfs are
magenta
• Adam Burrows et al
(2001) (520-603-3297)
• due to atmospheric
absorption by Sodium
and Potassium
David Bennett - Smallest Planet Orbits Smallest Star
Possibly a Low-Mass Red-Dwarf
Star
Future observations with
the Hubble Space
Telescope or the
European Southern
Observatory’s Very
Large Telescope will
decide this issue.
David Bennett - Smallest Planet Orbits Smallest Star
The Microlensing Method
• Uses a background star as
a source of light
• Gravitational field of star
and planet act as a lens
• requires no light from the
planetary host
• Observed signal is
changing magnification
• Required alignment is very
rare, so the very dense
Galactic bulge fields are
observed
David Bennett - Smallest Planet Orbits Smallest Star
Source Star Moves Across
Lens Magnification Pattern
Observed brightness changes as source star crosses lens system
magnification pattern. (credit: Fumio Abe, MOA Collaboration)
David Bennett - Smallest Planet Orbits Smallest Star
Observed Light Curve
• planetary signal
captured by MOA
• due to new wide
field-of-view
telescope and
camera
David Bennett - Smallest Planet Orbits Smallest Star
New MOA Telescope
Enabled Discovery
• 1.8m MOA-2 telescope
– Mt. John Observatory, NZ
• MOA-cam3 CCD Camera
– Images 2.2 sq. deg.
– 13 times the area of the full
moon
• Entire Galactic Bulge
imaged every hour
– All microlensing events
monitored for planets
• Similar telescopes are
needed in Chile (OGLEIV) and South Africa
David Bennett - Smallest Planet Orbits Smallest Star
Comparison to Other Exoplanets
steam at
t = 1 Myr
snow at
t = 1 Myr
Microlensing discoveries in red, transit discoveries in blue and Doppler discoveries
in black. Letters indicate Solar System planets. The snow-line relates to the
conditions
David Bennett - Smallest Planet Orbits Smallest Star
Credits & Further Info
for further info, contact David Bennett (cell phone: 574-315-6621)
or go to
http://www.nd.edu/~bennett/moa07blg192/
Scientific Paper to be published in the Astrophysical Journal (arXiv:0806.0025)
Authors:
D.P. Bennett1, I.A. Bond1, A. Udalski2, T. Sumi1, F. Abe1, A. Fukui1, K. Furusawa1,
J.B. Hearnshaw1, S. Holderness1, Y. Itow1, K. Kamiya1, A.V. Korpela1, P.M.
Kilmartin1, W. Lin1, C.H. Ling1, K. Masuda1, Y. Matsubara1, N. Miyake1, Y. Muraki1,
M. Nagaya1, T. Okumura1, K. Ohnishi1, Y.C. Perrott1, N.J. Rattenbury1, T. Sako1,
To. Saito1, S. Sato1, L. Skuljan1, D.J. Sullivan1, W.L. Sweatman1, P.J. Tristram1,
P.C.M. Yock1, M. Kubiak2, M.K. Szymanski2, G. Pietrzynski2, I. Soszynski2, O.
Szewczyk2, L. Wyrzykowski2, K. Ulaczyk2, V. Batista3, J.P. Beaulieu3, S. Brillant3,
A. Cassan3, P. Fouque3, P. Kervella, D. Kubas3, and J.B. Marquette3
1MOA Collaboration
2OGLE Collaboration
3PLANET Collaboration
US effort funded by the NSF and NASA
David Bennett - Smallest Planet Orbits Smallest Star