About site: Astronomy/Extrasolar Planets - Microvariability and Oscillations os STars
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  About site: http://www.astro.ubc.ca/MOST/

Title: Astronomy/Extrasolar Planets - Microvariability and Oscillations os STars Detection and characterisation of: (1) acoustic oscillations in Sun-like stars, including very old stars (metal-poor subdwarfs) and magnetic stars (roAp), to probe seismically their structures and age
Mid-InfraRed_Large-well_Imager MIRLIN - The JPL Deep-Well Mid-Infrared Array Camera

Nova_Celestia_-_A_Guide_to_Extrasolar_Planets Contains information and free illustrations of Extrasolar planets (carbon planets, gas giants and terrestrial planets), detection methods and missions.

The_Optical_Gravitational_Lensing_Experiment_(OGLE) A long term project with the main goal of searching for the dark matter with microlensing phenomena.

Optical_Long_Baseline_Interferometry_News NASA JPL's Optical Long Baseline Interferometer project homepage. Aims to increase optical resolution of the local universe sufficient to detect extrasolar planets and other phenomena.

The_Origin_of_Planetary_Systems_-_EU_Network Home site of European Union funded Research Training Network "The Origin of Planetary Systems".

Planet_Imager NASA planet imager proposal.


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MOST: Canada's First Space Telescope MOST logo MOST: Microvariability & Oscillations of STars - Microvariabilité & Oscillations STellaires Home Overview Project Milestones Partners Target Stars Science Galleries Links Canada's First Space Telescope
Le premier téléscope spatial Canadien Make MOST stand for "My Own Space Telescope". All Canadians - from students to amateur astronomers - are invited to submit science proposals for the MOST mission through this link, which contains information on MOST capabilities, a target selection tool, and an on-line proposal submission form. Start thinking of the science you might be able to do with Canada's space telescope. The MOST Science Team may choose your idea and work with you to analyse the data. MOST RECENT NEWS August 27th, 2008 MOST and NASA collaborate The Canadian Space Agency (CSA), NASA and the MOST Science Team have announced an agreement that will give U.S. researchers access to observing time with Canada’s MOST space telescope. MOST science target selection has been done exclusively by the MOST Science Team, with the support of CSA, and they have collaborated with members of the Canadian and international astronomical communities on some MOST observations. With this MOST NASA Guest Observer Program, up to 2 months of the science observation time during February 2009 through January 2010 will be made available to American astronomers. The submitted proposals will be evaluated and ranked by the MOST Science Team and three NASA-appointed scientists. They will seek out the best science proposals exploiting the unique capabilities of MOST. The final selection based on this ranking will be made by NASA’s Science Directorate. NASA will provide research funding to the Principal Investigators of the successful proposals. The high scientific value of the MOST satellite, since starting operations in 2003, has been well demonstrated and recognized widely throughout the international community. This new program illustrates the enduring collaboration between the Canadian and American space agencies, and opens up new scientific opportunities for the MOST mission to benefit an even broader research community. August 27th, 2008 THE SKY’S NOT THE LIMIT FOR CANADIANS - Amateur astronomers win time on the MOST space telescope Two Canadian amateur stargazers will trade in their backyard telescopes for one above their backyards... 820 kilometres above their backyards. Last year, the MOST team created an opportunity to make MOST mean "My Own Space Telescope". Amateur astronomers and students across Canada were invited to submit proposals for science to be done from orbit. The MOST Science Team has just selected the first two winners: David Gamey, from Toronto, who inspires his Scout packs to look to the stars, and Gordon Sarty, from Saskatoon, whose day job is to peer into the human brain. Read the full story. June 30th, 2008 NEW MOST RESULTS ON PROCYON RELEASED MOST's first primary science target was the bright star Procyon, observed in January 2004. MOST returned to Procyon the next year, and again last year during January - February 2007. The 2007 observing run returned the best photometry MOST had collected in its entire mission. The results have just been accepted for publication in The Astrophysical JOurnal, in a paper entitled "The nature of p-modes and granulation in Procyon: New MOST photometry and new Yale convection models" with lead author and MOST Science Team member Dr. David Guenther (St. Mary's University, Halifax). Collaborating on this research are Yale astronomers Frank Robinson and Pierre Demarque, who have generated numerical hydrodynamical 3D models of the turbulence in the atmosphere of the star Procyon for comparison with the MOST observations. Precise photometry of Procyon by the MOST satellite has generated debate over the nature of acoustic oscillations (p-modes) in that well-studied star. We present new photometry of Procyon obtained by MOST during a 38-day run in 2007 and frequency analyses of those data. The long time coverage and very low point-to-point scatter of the light curve yield an average noise amplitude of about 1.5 – 2.0 parts per million in the frequency range where p-modes are expected in Procyon. This is half the noise level obtained from each of the previous two Procyon campaigns by MOST in 2004 and 2005, thanks to enhanced satellite and instrument performance. The new data and theoretical models indicate that the dynamics of the atmosphere of a star like Procyon are more complicated than previously understood and different than what is seen in our Sun. The MOST spacebased photometry was obtained at the same time as a global multi-observatory campaign of spectroscopy to measure the oscillations of Procyon in radial velocity. The direct comparison of the two simultaneous data sets will almost certainly reveal even more insights into the nature of Sun-like stars. The new MOST paper is available on the Science page and the data are now available in the MOST Public Data Archive (through a link on the Science page). June 30th, 2008 HAPPY BIRTHDAY, MOST! MOST was launched five years ago today and the MOST Team is in a party mood. “After five years in space, MOST is making us feel like five-year-olds – curious, excited, and full of wonder at the new things we see every day,” said Dr. Jaymie Matthews, MOST Mission Scientist. “And while MOST is only five years old, it’s actually entering middle age, in a life of exploration that was supposed to last only twelve months.” The size of a suitcase, with a cost of only Can $10M, MOST was nicknamed by its creators the “Humble Space Telescope.” But its accomplishments have been anything but modest. It was originally intended to probe the hidden interiors of stars through their vibrations, by a technique called asteroseismology. “We’re literally listening to the music of the stars,” explains Matthews. “It’s like using a space telescope as an interstellar iPod.” MOST data have already turned up important – and sometimes controversial – results about the nature of stars, sending many theorists back to their computer screens to revise stellar models. MOST turned out to be a precocious child. The team of scientists and engineers – located from coast to coast across Canada and in Harvard and Vienna – has extended the capabilities of this ‘little telescope that could’ to explore exoplanets: alien worlds around other stars. MOST has measured the properties of several of these planets, which are invisible even to the largest telescopes. Among the findings: A planet whose atmosphere is either so clear or so hazy that it reflects only 4% of the light it receives from its parent sun. “Who could have imagined a planet darker than charcoal, whose sun is 400 times brighter in its sky than our Sun, except possibly a science fiction writer?” asks Matthews, “Well, MOST has turned us into real estate agents to science fiction and fantasy writers. The exoplanetary systems we are studying will be the settings of future novels and movies.”   PARTNERS Canadian Space Agency UBC Dept. of Physics and Astronomy
Mission Science Centre; Instrument Development Site; Ground Station Site; Primary Science Data Analysis Centre Dynacon UTIAS-SFL AMSAT CRESTech Spectral IfA, University of Vienna     An artist's rendering of MOST in orbit   MOST is a suitcase-sized (65 cm x 65 cm x 30 cm, 60 kg) microsatellite designed to probe stars and extrasolar planets by measuring tiny light variations undetectable from Earth. This can be done with such a small telescope (15 cm aperture) thanks to new Canadian attitude control technology. MOST - un microsatellite de la taille d'une mallette (65 cm x 65 cm x 30 cm, 60 kg), explorera étoiles et planètes extrasolaires en mesurant d'infimes variations de lumière indétectables depuis la Terre. L'utilisation d'un télescope de si petite taille (ouverture de 15 cm) est rendue possible grâce à la nouvelle technologie canadienne de commande d'attitude de satellites. FastCounter by bCentral
 

Detection

and

characterisation

of:

(1)

acoustic

oscillations

in

Sun-like

stars,

including

very

old

stars

(metal-poor

subdwarfs)

and

magnetic

stars

(roAp),

to

probe

seismically

their

structures

and

age

http://www.astro.ubc.ca/MOST/

Microvariability and Oscillations os STars 2008 December

dvd rental

dvd


Detection and characterisation of: (1) acoustic oscillations in Sun-like stars, including very old stars (metal-poor subdwarfs) and magnetic stars (roAp), to probe seismically their structures and age

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