Made famous in 1995 by NASA’s Hubble Space Telescope, the Pillars of Creation in the heart of the Eagle Nebula have captured imaginations worldwide with their arresting, ethereal beauty.
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Laboratory Characterization Of Hydrothermally Processed Oligopeptides In Ice Grains Emitted By Enceladus And Europa
The Cassini mission provided evidence for a global subsurface ocean and ongoing hydrothermal activity on Enceladus, based on results from Cassini’s mass spectrometers. Laboratory simulations of hydrothermal conditions on icy […]
A Dust-Trapping Ring in the Planet-Hosting Disk of Elias 2-24
Rings and gaps are among the most widely observed forms of substructure in protoplanetary disks.
Astrochemistry Update: Hubble Observes Infant Stars In Molecular Cloud RCW 7
This NASA/ESA Hubble Space Telescope image presents a visually striking collection of interstellar gas and dust. Named RCW 7, the nebula is located just over 5,300 light-years from Earth in […]
Chemistry Across Dust and Gas Gaps in Protoplanetary Disks: Modelling the Co-spatial Molecular Rings in the HD 100546 Disk
High-resolution observations show that typically both the dust and the gas in nearby extended protoplanetary disks are structured, possibly related to radial and azimuthal variations in the disk density and/or […]
The Solar System: Structural Overview, Origins and Evolution
Understanding the origin and long-term evolution of the Solar System is a fundamental goal of planetary science and astrophysics.
SPHERE RefPlanets: Search For Epsilon Eridani b And Warm Dust
We carried out very deep VLT/SPHERE imaging polarimetry of the nearby system Eps Eri based on 38.5 hours of integration time with a 600 – 900 nm broadband filter to […]
Astrogeology/Astrochemistry/Astrobiology Update: New Horizons Detects Dusty Hints Of An Extended Kuiper Belt
New observations from NASA’s New Horizons spacecraft hint that the Kuiper Belt – the vast, distant outer zone of our solar system populated by hundreds of thousands of icy, rocky […]
The Possibility Of Panspermia In The Deep Cosmos By Means Of The Planetary Dust Grains
By obtaining the assumption that planetary dust particles can escape from the gravitational attraction of a planet, we consider the possibility for the dust grains to leave the star’s system […]
chemcomp: Modeling The Chemical Composition Of Planets Formed In Protoplanetary Disks
Future observations of exoplanets will hopefully reveal detailed constraints on planetary compositions. Recently, we have developed and introduced chemcomp (Schneider & Bitsch 2021a), which simulates the formation of planets in […]
