A nearby M Star with tree Transitting Supter-Earths Discovered by K2

Small, cool planets represent the typical end-products of planetary formation. Studying the architectures of these systems, measuring planet masses and radii, and observing these planets' atmospheres during transit directly informs theories of planet assembly, migration, and evolution. Here we report the discovery of three small planets orbiting a bright (K-s = 8.6 mag) M0 dwarf using data collected as part of K2, the new ecliptic survey using the repurposed Kepler spacecraft. Stellar spectroscopy and K2 photometry indicate that the system hosts three transiting planets with radii 1.5-2.1 R-circle plus, straddling the transition region between rocky and increasingly volatile-dominated compositions. With orbital periods of 10-45 days the planets receive just 1.5-10x the flux incident on Earth, making these some of the coolest small planets known orbiting a nearby star; planet d is located near the inner edge of the system's habitable zone. The bright, low-mass star makes this system an excellent laboratory to determine the planets' masses via Doppler spectroscopy and to constrain their atmospheric compositions via transit spectroscopy. This discovery demonstrates the ability of K2 and future space-based transit searches to find many fascinating objects of interest.

PLANT MACROFOSSIL METHODS AND STUDIES | Treeline Studies

Macrofossil series from mountainous and polar areas such as the Alps, the Scandes, and the Rocky Mountains provide useful information about the late Quaternary course of treelines. Reconstructions of past treeline positions and compositions after the Ice Age can be used to infer paleoclimatic information or to study treeline ecosystem responses to (rapid) climatic change. Both approaches are illustrated by study cases. In addition to these paleoclimatic and paleoecological issues, macrofossil records can be used to validate dynamic treeline vegetation models. An example from the Alps shows the high potential of such a procedure towards applying forest-succession models for assessing future vegetation dynamics at treeline.