John B. Biersteker

TL;DR: In this paper, the authors compared photographs of the 2006 March 29 total eclipse with current-free extrapolations of photospheric field measurements and with images from the Solar and Heliospheric Observatory (SOHO) to deduce that the bulk of these linear features fall into three categories: (1) polar and low-latitude plumes that overlie small magnetic bipoles inside coronal holes, (2) helmet streamer rays that overlies large loop arcades and separate coronal hole of opposite polarity, and (3) pseudostreamer

TL;DR: It is shown that the atmospheric loss caused by these effects can significantly exceed that caused by mechanical shocks for hydrogen-helium (H/He) envelopes, and complete loss can occur when the impactor mass is comparable to the envelope mass.

TL;DR: In this paper, the WIS 91600 ungrouped C2 chondrite experienced an ancient field intensity of 4.4 ± 2.8 μT at ∼9.8 au, indicating that the parent body formed in the distal solar system, and the recovered formation distance argues that this body previously traveled from ∼10 au to 2-3 au, supporting the migration of asteroid-sized bodies throughout the solar system.

TL;DR: Ten recommendations for bolstering a data-rich future in planetary science from machine learning methods that expand the ability to construct, and draw insight from large datasets.

TL;DR: Icy moons around the ice giant planets may contain subsurface oceans, and their oceans could be detected and characterized using measurements of magnetic fields induced by the host planet's time-varying magnetic field as mentioned in this paper.