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I N T R O D U C T I O N T O
T R A P P I S T
T R A N S I T I N G P L A N E T S A N D P L A N E T E S I M A L S M A L L T E L E S C O P E
S . O . U . P
S T U D E N T S O F U N D E R G R A D U AT E P H Y S I C S
Lian Jia Yi SIF160094
Masmira Bt Masud SEB150012
Ang Yee Xiang SIF10012
Irene Ann Iype SIF160701
Koay Jing Wei SIF160092
Kanmalar Mathavan (SIF160026)
Pershaanaa A/P K. Manogran SIF160075
Nur Izzah Aqilah Bt Mat Said SIF160062
I N T R O D U C T I O N
• planetary system, located 12
parsecs away from solar system
near ecliptic, within the
constellation of Aquarius
• around a star( a red dwarf star),
which is 12 times less massive
than our sun, slightly larger than
Jupiter, there at least 7 planets
• planets have sizes and masses
comparable to earth
• at least 3 out of 7 planets are in
the habitable zone
T R A P P I S T- 0 1
A T R E A S U R E T R O V E O F P L A N E T S
F O U N D …
This artist's concept allows us to imagine what it would be like to
stand on the surface of the exoplanet TRAPPIST-1
M E T H O D O F D I S C O V E RY
M E T H O D 1 :
PA R A L L A X
• also known as stellar parallax
or trigonometric parallax
• a method used by
astronomers to calculate the
distance of star nearby to
the earth by using
trigonometry method
FORMULA USED :
TRIGNOMETRY
M E T H O D 2 :
S TA N D A R D
C A N D L E
• A second method of
measuring distance between
stars when parallax couldn’t
• Cepheid Variables
• Tully-Fisher Relation
• Very Long Baseline
Interferometry (VLBI)
• TypeIa Supernovae
• Sunyaev-Zeldovich Effect
• Gravitationally Lensed Quasars
C U R R E N T L I S T O F
S TA N D A R D C A N D L E S
M E T H O D 3 :
T R A N S I T
P H O T O M E T RY
• telescope watches a star for a period of time and records the amount
of light coming from the star.
• star is charted as a function of time.
• Look out for dips in the light curve which occur when planet blocks
light coming from star
K E P L E R ’ S
3 L A W S
O F
M O T I O N
The path of the planets about the
sun is elliptical in shape, with the
center of the sun being located
at one focus
T H E L A W O F
E L L I P S E S
An imaginary line drawn from the
center of the sun to the center of
the planet will sweep out equal
areas in equal intervals of time
T H E L A W O F
E Q U A L A R E A S
The ratio of the squares of the
periods of any two planets is
equal to the ratio of the cubes of
their average distances from the
sun
T H E L A W O F
H A R M O N I E S
S P R I T Z E R
S PA C E
T E L E S C O P E
• An infrared telescope that trails
Earth as it orbits the sun.
• It was well-suited for studying
TRAPPIST-1 because the star glows
brightest in infrared light, whose
wavelengths are longer than the
eye can see.
• Why did we launch it into space
instead of observing from Earth? (this
question can come out like a
popout. Ans in description)
• It has 3 science instruments that are cooled with liquid helium.
• It is not orbit around Earth-actually follows Earth’s orbit around the Sun and
doesn’t orbit Earth
• Because the instrument must be kept very cold, so it was best to keep it further
away from earth.
• This is because the telescope is trying to observe heat.
• If the telescope was warmer, the extra heat would overwhelm the faint IR
signals from space.
• The telescope must also be protected from heat of sun
• So it carriers a special solar shield and always points away from sun.
The End

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Trappist 01

  • 1. I N T R O D U C T I O N T O T R A P P I S T T R A N S I T I N G P L A N E T S A N D P L A N E T E S I M A L S M A L L T E L E S C O P E
  • 2. S . O . U . P S T U D E N T S O F U N D E R G R A D U AT E P H Y S I C S Lian Jia Yi SIF160094 Masmira Bt Masud SEB150012 Ang Yee Xiang SIF10012 Irene Ann Iype SIF160701 Koay Jing Wei SIF160092 Kanmalar Mathavan (SIF160026) Pershaanaa A/P K. Manogran SIF160075 Nur Izzah Aqilah Bt Mat Said SIF160062
  • 3. I N T R O D U C T I O N
  • 4. • planetary system, located 12 parsecs away from solar system near ecliptic, within the constellation of Aquarius • around a star( a red dwarf star), which is 12 times less massive than our sun, slightly larger than Jupiter, there at least 7 planets • planets have sizes and masses comparable to earth • at least 3 out of 7 planets are in the habitable zone T R A P P I S T- 0 1
  • 5. A T R E A S U R E T R O V E O F P L A N E T S F O U N D …
  • 6.
  • 7.
  • 8.
  • 9. This artist's concept allows us to imagine what it would be like to stand on the surface of the exoplanet TRAPPIST-1
  • 10. M E T H O D O F D I S C O V E RY
  • 11. M E T H O D 1 : PA R A L L A X
  • 12. • also known as stellar parallax or trigonometric parallax • a method used by astronomers to calculate the distance of star nearby to the earth by using trigonometry method
  • 14. M E T H O D 2 : S TA N D A R D C A N D L E
  • 15. • A second method of measuring distance between stars when parallax couldn’t
  • 16.
  • 17. • Cepheid Variables • Tully-Fisher Relation • Very Long Baseline Interferometry (VLBI) • TypeIa Supernovae • Sunyaev-Zeldovich Effect • Gravitationally Lensed Quasars C U R R E N T L I S T O F S TA N D A R D C A N D L E S
  • 18. M E T H O D 3 : T R A N S I T P H O T O M E T RY
  • 19. • telescope watches a star for a period of time and records the amount of light coming from the star. • star is charted as a function of time. • Look out for dips in the light curve which occur when planet blocks light coming from star
  • 20. K E P L E R ’ S 3 L A W S O F M O T I O N
  • 21. The path of the planets about the sun is elliptical in shape, with the center of the sun being located at one focus T H E L A W O F E L L I P S E S
  • 22. An imaginary line drawn from the center of the sun to the center of the planet will sweep out equal areas in equal intervals of time T H E L A W O F E Q U A L A R E A S
  • 23. The ratio of the squares of the periods of any two planets is equal to the ratio of the cubes of their average distances from the sun T H E L A W O F H A R M O N I E S
  • 24. S P R I T Z E R S PA C E T E L E S C O P E
  • 25. • An infrared telescope that trails Earth as it orbits the sun. • It was well-suited for studying TRAPPIST-1 because the star glows brightest in infrared light, whose wavelengths are longer than the eye can see. • Why did we launch it into space instead of observing from Earth? (this question can come out like a popout. Ans in description)
  • 26. • It has 3 science instruments that are cooled with liquid helium. • It is not orbit around Earth-actually follows Earth’s orbit around the Sun and doesn’t orbit Earth • Because the instrument must be kept very cold, so it was best to keep it further away from earth. • This is because the telescope is trying to observe heat. • If the telescope was warmer, the extra heat would overwhelm the faint IR signals from space. • The telescope must also be protected from heat of sun • So it carriers a special solar shield and always points away from sun.
  • 27.