Results 201 to 210 of about 15,081 (214)

First direct observations of atmospheric sputtering at Mars. [PDF]

Sci Adv
Curry SM, Hara T, Luhmann JG, Leblanc F, Jolitz R, Mitchell D, Modolo R, Brain DA, Espley J, Benna M, Halekas J.   +10 more
europepmc   +1 more source

The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth. [PDF]

Life (Basel)
Kuzucan A, Bolmont E, Chaverot G, Ferreira JQ, Ibelings BW, Bhatnagar S, McGinnis DF.   +6 more
europepmc   +1 more source

A future classroom lab with active and gamified STEAM proposal for mathematics and science disciplines: Analyzing the effects on pre-service teacher's affective domain. [PDF]

Heliyon
Montero-Izquierdo AI, Jeong JS, González-Gómez D.   +2 more
europepmc   +1 more source

Astronomy from the Moon: the next decades (part 2). [PDF]

Philos Trans A Math Phys Eng Sci
Silk J, Crawford I, Elvis M, Zarnecki J.
europepmc   +1 more source

A qualitative assessment of limits of active flight in low density atmospheres. [PDF]

Sci Rep
Pajusalu M, Seager S, Huang J, Petkowski JJ.   +3 more
europepmc   +1 more source

Adaptive median filter salt and pepper noise suppression approach for common path coherent dispersion spectrometer. [PDF]

Sci Rep
Guan S, Liu B, Chen S, Wu Y, Wang F, Liu X, Wei R.   +6 more
europepmc   +1 more source

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Exoplanet Habitability

Science, 2013
The search for exoplanets includes the promise to eventually find and identify habitable worlds. The thousands of known exoplanets and planet candidates are extremely diverse in terms of their masses or sizes, orbits, and host star type. The diversity extends to new kinds of planets, which are very common yet have no solar system counterparts.
openaire   +2 more sources

The Worlds of Exoplanets

2018
The landscapes of exoplanets are likely to be incredibly diverse: exoplanets come in a large range of sizes and masses, and therefore surface gravities. Atmospheres can be thick layers, or absent. The interior makeup of exoplanets is even harder to know, but the formation scenarios of the giant planets and the remains of planets found in white-dwarf ...
openaire   +1 more source

The Architecture of Exoplanets

Space Science Reviews, 2016
Prior to the discovery of exoplanets our expectations of their architecture were largely driven by the properties of our solar system. We expected giant planets to lie in the outer regions and rocky planets in the inner regions. Planets should probably only occupy orbital distances 0.3–30 AU from the star.
openaire   +2 more sources