| Exoplanetary Scratchpad|
Systems Containing Planets Detected with TTV
- Kepler-9 System - Contains the 6th planet found by Kepler and the first star containing multiple transiting planets. The first system where transit times noted to vary due to interaction between planets, pioneering the transit timing variations method of confirmation. Has a hot Super-Earth that could be used to test the core accretion theory and two Saturn-sized planets. The two giant planets could have pushed the super Earth towards the star, which was unable to get the gasses needed form a Jupiter sized planet as the dust near the star rapidly dispersed.
- WASP-3 System - One of three systemss discovered by Super WASP containing a transiting planet so close to its star that it is evaporating. Like the other two, WASP-4 and 5, it is incapable of radiating away heat from its star and instead swells up to significantly larger than Jupiter. This is a planet 81% more massive than Jupiter with 13% larger radius going around in just less day 2 days. Its transit time varies by up to 3 minutes, which indicates that a further planet may be in this system. This would be a further Neptunian planet and would be the first exoplanet detected by measuring eclipse timing deviations of an earlier discovered planet (Transit Timing Variation method). Further observations are needed to confirm the planet, but the best fit is that it is in 2:1 resonance with the larger planet.
- WASP-5 System - One of three systems discovered by Super WASP containing a transiting planet so close to its star that it is evaporating. Found to orbit in the same manner as its star's rotation, while 6 out of 27 planets analyzed by the WASP team were found to orbit backwards around its star in 2010. Has a candidate planet detected by the Transit Timing Variation method.
- WASP-10 System - System that contains a super Jupiter around an orange star. At first believed to be inflated, but later found to be smaller. Has a density similar to the moon. Has a candidate planet detected by the Transit Timing Variation method.
- Kepler-19 System - System with two exoplanets discovered by Kepler, 690ly away. Planet b is a small Neptunian about 20 Earth masses and 2 Earth radii. It takes about 9 days to go around its star and has a surface temperature of 480C. Outer Planet c was discovered based on differences in transit timing (5 minutes) that it caused for Planet b. It is tilted relative to 'b', so it itself never transits. It is not massive enough to have its mass estimated. It could be a rocky planet on a circular 5-day orbit or a gas giant in an oblong 100 day orbit. First TTV detected planet confirmed that doesn't transit due to the fact that Kepler continuously observes the planet's transits, rather than stitches together several observations. Future observations with HARPs using radial velocity method will be used to pinpoint planet c's mass.