Results 141 to 150 of about 1,099 (180)

Strong link between Earth's oxygen level and geomagnetic dipole revealed since the last 540 million years. [PDF]

Sci Adv
Kuang W, Kopparapu R, Krissansen-Totton J, Mills BJW.   +3 more
europepmc   +1 more source

Tracing the inner edge of the habitable zone with sulfur chemistry. [PDF]

Sci Adv
Jordan S, Shorttle O, Rimmer PB.
europepmc   +1 more source

Slowing planetary rotation influences ocean nutrient cycling and oxygenation. [PDF]

Sci Adv
Capirala A, Olson SL.
europepmc   +1 more source

A hot-Jupiter progenitor on a super-eccentric retrograde orbit. [PDF]

Nature
Gupta AF, Millholland SC, Im H, Dong J, Jackson JM, Carleo I, Libby-Roberts J, Delamer M, Giovinazzi MR, Lin ASJ, Kanodia S, Wang XY, Stassun K, Masseron T, Dragomir D, Mahadevan S, Wright J, Alvarado-Montes JA, Bender C, Blake CH, Caldwell D, Cañas CI, Cochran WD, Dalba P, Everett ME, Fernandez P, Golub E, Guillet B, Halverson S, Hebb L, Higuera J, Huang CX, Klusmeyer J, Knight R, Leroux L, Logsdon SE, Loose M, McElwain MW, Monson A, Ninan JP, Nowak G, Palle E, Patel Y, Pepper J, Primm M, Rajagopal J, Robertson P, Roy A, Schneider DP, Schwab C, Schweiker H, Sgro L, Shimizu M, Simard G, Stefánsson G, Stevens DJ, Villanueva S, Wisniewski J, Will S, Ziegler C.   +59 more
europepmc   +1 more source

Ionic Liquid Biospheres. [PDF]

Life (Basel)
Seager S, Bains W, Iakubivskyi I, Agrawal R, Jenkins J, Shinde P, Petkowski JJ.   +6 more
europepmc   +1 more source

Warm, water-depleted rocky exoplanets with surface ionic liquids: A proposed class for planetary habitability. [PDF]

Proc Natl Acad Sci U S A
Agrawal R, Seager S, Iakubivskyi I, Buchanan WP, Glidden A, Seager MD, Bains W, Huang J, Petkowski JJ.   +8 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Exoplanet Formation

2022
Madhu Kashyap Jagadeesh, Usha Shekhar
exaly   +2 more sources

Atmospheric signatures of giant exoplanet formation by pebble accretion [PDF]

Monthly Notices of the Royal Astronomical Society, 2017
Atmospheric chemical abundances of giant planets lead to important constraints on planetary formation and migration. Studies have shown that giant planets that migrate through the protoplanetary disc can accrete substantial amounts of oxygen-rich planetesimals, leading to supersolar metallicities in the envelope and solar or subsolar C/O ratios. Pebble
Nikku Madhusudhan, Anders Johansen, Bertram Bitsch   +2 more
exaly   +3 more sources

Directly imaged exoplanet challenges formation models

Physics Today, 2010
Stephen G Benka
exaly   +2 more sources

Formation and Evolution of Exoplanets

2010
Introduction Exoplanet Observations Pinpointing Planets in Circumstellar Disks Planet-Planet Interactions Formation via Disk Instability Core Accretion Model Formation of Terrestrial Planets Brown Dwarfs Exoplanet Chemistry Migration and Multiplicity Effects During Giant Planet formation Planets in mean motion resonance Planet-Planet Gravitational ...
openaire   +1 more source