Hot super-Earths stripped by their host stars.

Simulations predict that hot super-Earth sized exoplanets can have their envelopes stripped by photoevaporation, which would present itself as a lack of these exoplanets. However, this absence in the exoplanet population has escaped a firm detection. Here we demonstrate, using asteroseismology on a sample of exoplanets and exoplanet candidates observed during the Kepler mission that, while there is an abundance of super-Earth sized exoplanets with low incident fluxes, none are found with high incident fluxes. We do not find any exoplanets with radii between 2.2 and 3.8 Earth radii with incident flux above 650 times the incident flux on Earth. This gap in the population of exoplanets is explained by evaporation of volatile elements and thus supports the predictions. The confirmation of a hot-super-Earth desert caused by evaporation will add an important constraint on simulations of planetary systems, since they must be able to reproduce the dearth of close-in super-Earths.

Ensemble asteroseismology of solar-type stars with the NASA Kepler mission.

In addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solar-type stars in the Kepler field of view, an ensemble that is large enough to allow statistical studies of intrinsic stellar properties (such as mass, radius, and age) and to test theories of stellar evolution. We find that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.

Kepler detected gravity-mode period spacings in a red giant star.

Stellar interiors are inaccessible through direct observations. For this reason, helioseismologists made use of the Sun's acoustic oscillation modes to tune models of its structure. The quest to detect modes that probe the solar core has been ongoing for decades. We report the detection of mixed modes penetrating all the way to the core of an evolved star from 320 days of observations with the Kepler satellite. The period spacings of these mixed modes are directly dependent on the density gradient between the core region and the convective envelope.

Ethylene response to pollen tube growth in Nicotiana tabacum flowers.

In flowers of Nicotiana tabacum L., pollination induces a transient increase in ethylene production by the pistil. The characteristic dynamics of the increase in ethylene correspond to the main steps of the pollen-tube journey into the pistil: penetration into the stigma, growth through the style, entry into the ovary and fertilization. Ethylene is synthesized de novo in the pistil, and its production is reduced in the dark. Ethylene production was monitored in tobacco flowers after pollination with incongruous pollen from three different Nicotiana species, N. rustica, N. repanda and N. trigonophylla, and with pollen from Petunia hybrida. Pollen from all of these different sources can germinate on the stigma surface but each pollen type shows a different behavior and efficiency in penetrating the pistil tissues. Thus, these different crosses provided a model with which to study the response of the pistil to pollination and fertilization. Ethylene evolution upon pollination in tobacco differed in each cross, suggesting that ethylene is correlated with the response to pollen tube growth in the tobacco flower.