Astrobiology33- Page

MUSE and NIRCam images of d203-504 environment. Left: MUSE NFM composite image of both d203-506 (bottom left) and d203-504 (top). Red: the (λ8727˚A) map showing disk contributions from both

By delving into ancient rock records, scientists have uncovered new clues that sharpen the timeline of Earth’s oxygenation—shedding fresh light on one of the most transformative chapters in our planet’s

Taken on 28 May 2025, this image of the preparative zone of cultured tobacco cells with visualized microtubules (yellow: microtubules , magenta: nuclei). For the Effects of the Space

Numerical simulations of lava planets interior dynamics with no rotation. The dimensionless temperature scale is the maximum super-adiabatic temperature contrast: temperature is 1 at the base of the magma ocean,

Ocean World – Grok via Astrobiology.com Future missions to icy ocean worlds (OW) such as Europa and Enceladus will evaluate the habitability and potential for biosignatures on these worlds. These

External components on the TISR return vehicle. — NASA NTRS Titan is unique in the outer solar system in that it is the only moon with a thick atmosphere, and

The magnification excess maps for planet-satellite configurations with log q = −1.5 and | log s| = 0.3. The color coding indicates fractional magnification differences between the 2L1S and 1L1S

Graphical Abstract — Earth, Planets and Space via X-mol The formation and alteration of organic molecules within the Solar System and beyond is closely related to the life cycle of

Normalised to peak flux spectra of our sample of millimetre-compact disks. The red line indicates the estimated continuum. The indicated types and their meaning are discussed in Section 5.1. In

Schematic overview of CO2 ice segregation in protostellar envelopes. The temperature and density zones are separated by the gray dashed lines and each grain represents a different stage of ice