...118, 49, 677, and 5700 days, and minimum masses of 0.63, 0.17, 0.1, 0.05, 0.12 and 0.38 (compared with Jupiter) respectively. All of the planets were found via the radial-velocity method. This method is often to referred to as the ‘wobble’ method and...
... line between super-Earth (rocky) and sub-Neptune (somewhat gassy) planets; planet b has a radii of 1.64, planet c is 1.29 and planet d is 2.08. Using their Planet Finding Spectrograph (PFS) to monitor GJ 9827, the team which is headed by Johanna...
...orbital period is about 12 years, Saturn’s is 29 years and Uranus completes its orbital period once in a human lifetime. Planet X on the other hand, which is postulated to be 60 billion miles from the Sun, is expected to take 20,000 years to complete...
...been found, interest in the existence of a hypothesised Planet Nine has been reignited over the years, more recently ... of TNOs in conjunction with the orbits of the giant outer planets but instead of calculating the contents of the Kuiper Belt as ...
... Rubin Observatory will produce," Bernardinelli says. The searches could also help determine whether Planet Nine, a hypothesised Neptune-sized planet that's thought to inhabit space beyond Pluto, really exists or not. "There are lots of ideas...
... instrument called SOPHIE installed at the Haute-Provence Observatory in the South of France, astronomers have discovered a six planet system containing a "super-Earth" and five "mini-Neptunes,” all with exceptionally regular spacing; a feature which...