Astrochemistry
Modeling Complex Organic Molecules in Dense Regions 
Recent observations have revealed the existence of Complex Organic Molecules (COMs) in cold dense cores and prestellar cores.
Extrasolar Planets
Making Planets in the Laboratory
New laser-driven compression experiments reproduce the conditions deep inside exotic super-Earths and giant planet cores, and the conditions during the violent birth of Earth-like planets, documenting the material properties that determined planets' formation and evolution processes.
Polar Research
Where Ice sheet, Ocean and Land Converge
Using a specially designed hot-water drill to cleanly bore through a half mile of ice, a National Science Foundation (NSF)-funded team of researchers has become the first ever to reach and sample the "grounding zone," where Antarctic ice, land and sea all converge.
Extrasolar Planets
Nearby M Star With Three Transiting Super-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.
Habitable Zones & Global Climate
Extrasolar Planets Are More Hospitable to Life Than Previously Thought
A study by astrophysicists at the University of Toronto suggests that exoplanets - planets outside our solar system - are more likely to have liquid water and be more habitable than we thought.
Astrobiology (general)
In Memoriam: Antonio Behar
The Astrobiology community deeply mourns the loss of Dr. Antonio Behar, a JPL employee, explorer, colleague, and friend to many. He died in the crash of a small plane on Friday, January 10, 2015, near Van Nuys Airport in the Los Angeles area.
Extrasolar Planets
Ammonia, Water Clouds and Methane Abundances of Giant Exoplanets and Opportunities for Super-Earth Exoplanets
Future direct-imaging exoplanet missions such as WFIRST/AFTA, Exo-C, and Exo-S will measure the reflectivity of exoplanets at visible wavelengths.
Astrochemistry
Infrared Spectra and Chemical Abundance of Methyl Propionate in Icy Astrochemical Conditions
We carried out an experiment in order to obtain the InfraRed (IR) spectra of methyl propionate (CH3CH2COOCH3) in astrochemical conditions and present the IR spectra for future identification of this molecule in the InterStellar Medium (ISM).
Extrasolar Planets
Planet Formation in Post-common-envelope Binaries
To understand the evolution of planetary systems, it is important to investigate planets in highly evolved stellar systems, and to explore the implications of their observed properties with respect to potential formation scenarios.
Astrochemistry
Search for Methylamine in High Mass Hot Cores
We aim to detect methylamine, CH3NH2, in a variety of hot cores and use it as a test for the importance of photon-induced chemistry in ice mantles and mobility of radicals.
Extrasolar Planets
Planetary Systems in Star Clusters
In the solar neighborhood, where the typical relaxation timescale is larger than the cosmic age, at least 10% to 15% of Sun-like stars have planetary systems with Jupiter-mass planets. In contrast, dense star clusters, charactered by frequent close encounters, have been found to host very few planets.
More top stories from January.
Recent Releases
Recent Status Reports
Calendar
- 29 Jan: Delta II Launch of NASA's Soil Moisture Active Passive (SMAP)
- 29 Jan: SESE New Discoveries Lecture Series: Building Earth-like planets
- 30 Jan: Queen's Space Conference
- 2 Feb: Icy Worlds Media Day
- 4 Feb: Workshop on Early Solar System Bombardment III
- 4 Feb: FAA Commercial Space Transportation Conference
- 8 Feb: SpaceX Falcon 9 Launch of DSCOVR
- 11 Feb: Arianespace Launch of the ESA Intermediate eXperimental Vehicle (IXV) on a Vega Rocket
- 11 Feb: Aerospace Safety Advisory Panel Meeting
- 12 Feb: STA Reception for Chairman Lamar Smith and Chairman Steve Palazzo
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