M dwarf – Astronomy Now

Potentially habitable super-Earth is a prime target for atmospheric study

20 April 2017 Astronomy Now

The study of alien worlds is entering its next phase as astronomers amass the best planets outside our Solar System to look for signs of life. A newly discovered “super-Earth” orbiting in the habitable zone of a nearby small star, has catapulted itself to the top of that list.

Possible Venus twin discovered around dim star

11 April 2017 Astronomy Now

Astronomers using NASA’s Kepler space telescope have found a planet 219 light-years away that seems to be a close relative to Venus. This newly discovered world is only slightly larger than Earth and orbits a low-temperature star called Kepler-1649 that’s one-fifth the diameter of our Sun.

Potentially habitable super-Earth K2-3d observed transiting parent star

28 November 2016 Astronomy Now

A group of researchers has observed the first ground-based transit observation of K2-3d — a potentially Earth-like extrasolar planet supposedly within the habitable zone around a bright M-dwarf host star 147 light-years away — using the multi-band imager MuSCAT on the Okayama Astrophysical Observatory’s 1.88-metre telescope.

Oldest known planet-forming circumstellar disc discovered

22 October 2016 Astronomy Now

A group of citizen scientists and professional astronomers joined forces to discover an unusual hunting ground for exoplanets. They found a red dwarf, called AWI0005x3s, surrounded by the oldest known circumstellar disc — a 45-million-year-old primordial ring of gas and dust orbiting the star from which planets can form.

NASA’s Kepler space telescope confirms 100+ exoplanets during its K2 mission

19 July 2016 Astronomy Now

More than 100 confirmed exoplanets — the biggest haul of worlds uncovered by the stabilised and repurposed Kepler space telescope in its K2 mission — is reported by an international science team led by the University of Arizona. Excitingly, the new population includes many worlds that could be rocky and cool enough to potentially support life.

Stifling atmospheres could limit number of habitable exoplanets

26 May 2016 Astronomy Now

New research reveals that fewer than predicted planets may be capable of harbouring life because their atmospheres keep them too hot. Computer simulations show that planets similar to or larger in mass than the Earth that are born with thick envelopes of hydrogen and helium are likely to retain their stifling atmospheres.