All are orbited by white dwarfs with
orbital periods ranging from 4 to 27 hours.
The expected Doppler signals are too small to confirm them by demonstrating that their masses are in the planetary regi... ▽ More We present an investigation of twelve candidate transiting planets from Kepler with
orbital periods ranging from 34 to 207 days, selected from initial indications that they are small and potentially in the habitable zone (HZ) of their parent stars.
Not exact matches
In these cases, astronomers can reliably determine their short
orbital periods,
ranging from hours to days to a couple years.
Periods of volcanism can cool the climate (as with the 1991 Pinatubo eruption), methane emissions from increased biological activity can warm the climate, and slight changes in solar output and
orbital variations can all have climate effects which are much shorter in duration than the ice age cycles,
ranging from less than a decade to a thousand years in duration (the Younger Dryas).
Modern research have further confirmed that: (1) the planetary
orbital periods can be approximately deduced from a simple system of resonant frequencies; (2) the solar system oscillates with a specific set of gravitational frequencies, and many of them (e.g. within the
range between 3 yr and 100 yr) can be approximately constructed as harmonics of a base
period of ∼ 178.38 yr; (3) solar and climate records are also characterized by planetary harmonics from the monthly to the millennia time scales.