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EXTRASOLAR PLANETARY SYSTEMS DETECTION METHODS, RESULTS AND PERSPECTIVES MICHAŁ RÓŻYCZKA NICOLAUS COPERNICUS ASTRONOMICAL CENTER 1 ST PLANETS SHOOL, HEIDELBERG, OCT. 8 TH , 2003. AN EASY INTRODUCTION FOR EVERYBODY. The f irst discoveries Observ ing planet formation
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EXTRASOLAR PLANETARY SYSTEMS DETECTION METHODS, RESULTS AND PERSPECTIVES MICHAŁ RÓŻYCZKA NICOLAUS COPERNICUS ASTRONOMICAL CENTER 1STPLANETS SHOOL, HEIDELBERG, OCT. 8TH, 2003 AN EASY INTRODUCTION FOR EVERYBODY
The first discoveries • Observing planet formation • Detecting „mature” planets • Statistics of extrasolar systems • Future space missions
THE FIRST DISCOVERIES
1ST EXTRASOLAR PLANETARY SYSTEM ANNOUNCED IN JANUARY 1992 ALEX WOLSZCZAN 2 PLANETS (NOW 3) 1600 LIGHT YEARS FROM THE SUN CONSTELLATION VIRGO
A B C PSR 1257+12 DISTANCE (EARTH = 1) SUN MERCURY VENUS EARTH
A B C PSR 1257+12 DISTANCE (EARTH = 1) SUN MERCURY VENUS EARTH
... BUT PROMISING CERTAINLY GLORIOUS... ... BUT RATHERUNFRIENDLY THE FIRST EXTRASOLAR SYSTEM: SURPRISING
1ST PLANET AT A SOLAR-LIKE STAR ANNOUNCED IN OCTOBER 1995 MICHEL MAYOR DIDIER QUELOZ LONG BEFORE THAT STARBIRTH-PROCESSES HAVE BEEN STUDIED, YIELDING CLUES ABOUT PLANET FORMATION STAR 51 PEGASI 40 LIGHT YEARS FROM THE SUN CONSTELLATION PEGASUS
OBSERVING PLANET FORMATION (INDIRECTLY)
25 000 LIGHT YEARS 1011 STARS
CO, 2.64 mm 3-6×109 M 300 l.y. 3×105 M mostly H2 INFRARED CO
ORION NEBULA ORION STAR-FORMING REGION
VISIBLE INFRARED 2.5 l.y.
ORIONNEBULA AGE: A FEW MILLION YEARS 150 objects R = 50 -1000 AU M > 600 M (H2 emission; absorption of visible light emitted by the nebula )
b Pictoris AGE: 108 years dust mass: 0.1 M gas mass: 100 M Infrared 1,2m resolution 0,12’’ 63 l.y. 1.7 M 50 AU
DETAILS OF DISC DISPERSAL UNKNOWN DETAILS OF STAR AND DISC FORMATION UNKNOWN THE DISCS DISPERSE WITHIN ~ 107 YEARS STARS ARE BORN WITH CIRCUMSTELLAR DISCS
RESIDUAL DISCS SEEM TO CONTAIN MORE THAN JUST DUST
A PLANET? WARP b Pictoris
HOLE INNER PLANET(S)? OUTER PLANET? WARP AGE: 108 years dust mass:0.1 M FOMALHAUT 25 l.y. 2.8 M HOLE OUTER PLANET
INDIRECT EVIDENCE: RESIDUAL DISCS CONTAIN PLANETS
DETECTING MATURE PLANETS
JUPITER SHINES WEAKER THAN THE SUN: 1 000 000 000 TIMES(visible light) 50 000 TIMES(infrared) 5 000 TIMES(mm and sub-mm)
JUPITER OBSERVED FROM THE NEAREST STAR 0.1” DISTANT FROM THE SUN „DROWNED” IN SUNSHINE !! PSF, SEEING, ZODIACAL LIGHT, BACKGROUD SKY REMNANT DISK
AND YET WITHIN THE LAST 8 YEARS MORE THAN 110 EXTRASOLAR PLANETS HAVE BEEN FOUND HOW ??
POPULAR VIEW
POPULAR VIEW
REALITY X = CENTER OF MASS SYSTEM VIEWED POLE-ON (RARE)
REALITY SYSTEM VIEWED OBLIQUELY (MORE COMMON)
THE PLANET CANNOT BE SEEN ...BUT MOTIONS OF THE STAR BETRAY ITS PRESENCE !
450 km 9 cm/s 150 000 000 km 30 km/s X 750 000 km 13 m/s JUPITER X 780 000 000 km 13 km/s EARTH
2020 1995 2010 1990 2015 2005 2000 0.002” MOTIONS OF THE SUN VIEWED FROM A STAR 30 LIGHT YEARS AWAY 0.002’’ IS THE ANGULAR SIZE OF A MAN ON THE MOON OR A STANDARD NEWSPAPER FONT 300 KM AWAY
STELLAR WOBBLE RECEDING: REDDER APPROACHING: BLUER
to the observer i normal to the orbit 100 P m/s 50 K 0 -50 V -100 days 0 1 2 3 PLANET DETECTION DUE TO STELLAR WOBBLE K = Vsin i
MK/(sin iVPL) K= Vsin i PLANET DETECTION DUE TO STELLAR WOBBLE MPLsin i = MK/ VPL
KNOWN: • ORBITAL PERIOD • AMPLITUDE OF VELOCITY VARIATIONS • MASS OF THE STAR * COMPUTED: • MASS OF THE PLANET (LOWER LIMIT) • ORBITAL RADIUS
ANOTHER EFFECT: TRANSIT PLANET IN FRONT OF THE STAR
TRANSIT LIGHT CURVE 1% BRIGHTNESS TIME
FIRST DETECTION OF A PLANET VIA THE TRANSIT PHENOMENON ANNOUNCED IN 2002/2003 ANDRZEJ UDALSKI MACIEJ KONACKI STAR OGLE-TR-56 ~5000 LIGHT YEARS FROM THE SUN CONSTELLATION SAGITTARIUS
KNOWN: • ORBITAL PERIOD • AMPLITUDE OF VELOCITY VARIATIONS • MASS OF THE STAR • LIGHT CURVE • COMPUTED: • MASS OF THE PLANET (LOWER LIMIT) • RADIUS AND SHAPE OF THE ORBIT • COMPUTED: • MASS OF THE PLANET • RADIUS AND SHAPE OF THE ORBIT • RADIUS OF THE PLANET
BASIC STATISTICS OF EXTRASOLAR PLANETS