[Kyushu University] Planetary systems like our solar system are born within a disk of gas and dust (protoplanetary disk) surrounding a newly formed star. Observations with the ALMA telescope have […]
Astrogeology
Capture of Interstellar Planetesimals in Protoplanetary Discs in Binary Star Systems
[astro-ph.EP] Planet formation requires growth over 12 orders of magnitude in size, from micron-sized dust grains to fully formed planets.
Excess Oxygen Stored In Deep Earth Magma May Help Explain How Earth’s Atmosphere Became Oxygen-rich
[Science China Press] The research team, led by Dr. Yanhao Lin and Dr. Ho-kwang Mao of the Center for High Pressure Science and Technology Advanced Research (HPSTAR), together with Prof. […]
3D Global Climate Simulations of Synthetic Mars Warming
[astro-ph.EP] Artificial warming via engineered aerosols presents a novel pathway to bypass volatile scarcity on modern Mars.
ALMA Reveals Planetary Formation Structures In Small Disks
[ALMA] Thanks to the extraordinary sharpness of ALMA’s images, a research team has discovered rings, grooves, and cavities in extremely compact disks surrounding young stars.
Simulations Of The Evolving Ozone Layer: Implications For The Early Earth, Exoplanets, And The Search For Life
[astro-ph.EP] Over 4 billion years, Earth’s atmosphere has been transformed from a composition devoid of molecular oxygen (O2) to one where O2 is now 21% of our modern atmosphere by […]
A Proposal To Make Mars Sample Return A Collaborative NASA, ESA, And CNSA Effort
[Astrobiology (Journal) via PubMed] Humanity’s self-awareness drives the quest to understand the origins of life. Although Earth history has erased much of our planet’s early biological evidence, Mars preserves ancient […]
Planetary Research Program Metrics to Enable a Vital Research Community and Achieve Decadal-Level Science
[National Academies of Sciences] Help us identify ways that the NASA Planetary Research Program can evaluate the health and effectiveness of its research and analysis program in accomplishing decadal science […]
How Long Could Volcanic Plumes Persist In The Venus Atmosphere?
[astro-ph.EP] Resolving the ambiguity surrounding current Venusian volcanism is a primary objective for upcoming missions like EnVision and VERITAS.
“Mega-Earths” Are Likely An Artifact Of Stellar Activity
[astro-ph.EP]. Empirical relations and planet formation simulations suggest an upper mass limit for rocky planets of ∼10M⊕, as cores above this will almost certainly undergo runaway gas accretion.
