Could Alien Civilizations Build Dyson Bubbles? Scientists Say Stability Might Be Achievable

Life’s capacity to survive in simulated lunar and Martian soils has been explored in two papers published in Scientific Reports. Treating simulated lunar soil with both symbiotic fungi and worm-produced compost can significantly improve the likelihood of reproduction for chickpea plants growing in the soil, indicates one study. A separate paper suggests that some microbes may be able to absorb enough water from the atmosphere to grow in simulated Martian soil at atmospheric humidity levels comparable to those on the planet.

Lunar soil—known technically as lunar regolith —does not support healthy plant growth, as it contains high concentrations of certain metals such as aluminum and zinc, does not allow water to filter through easily, and lacks the microbiome found in Earth soils. Previous research has investigated several ways to improve the fertility of lunar soil, although plants grown in these treated soils typically display various signs of stress, including stunted growth and leaf yellowing.

Jessica Atkin and colleagues grew chickpea plants (Cicer arietinum) in samples of simulated lunar soil that they treated in two ways: by adding vermicompost —produced by red wiggler earthworms (Eisenia fetida) as they decompose biowaste—at different concentrations; and by inoculating half of the soil samples at each concentration with arbuscular mycorrhizal fungi (AMF). On Earth, AMF improve the nutrient circulation properties of soil, reduce the quantity of potentially toxic metals available for absorption by plants, and produce a protein that helps bind soil together to reduce erosion. The authors then measured the quantity and weight of chickpea seeds produced, along with the plants’ heights and root mass.

Researchers at Nagoya University in Japan have conducted the most detailed simulation of the interior of stars and disproved a theory scientists have believed for 45 years: that stars switch their rotation patterns as they age, with poles rotating faster than the equator in older stars. Scientists have now found that this switch may not occur. Stars maintain solar-type rotation, spinning fast at the equator and slow at the poles throughout their lifetime. The findings are published in Nature Astronomy.

Stars come in many different sizes, temperatures, and colors, ranging from red dwarfs to massive blue giants. Solar-type stars, the focus of this study, are those similar to our sun in mass and temperature. They are medium-sized, yellow stars that provide stable conditions for billions of years, long enough for planets orbiting them to potentially develop life.

Earth rotates as one solid piece, but because the sun is made of hot gas, it rotates differentially —different parts rotate at different speeds. The equator takes about 25 days to complete one rotation while the poles take about 35 days. This is known as solar-type differential rotation.

A new study challenges the traditional boundaries of the habitable zone, showing that liquid water could exist on the dark sides of tidally locked planets or beneath thick ice on distant worlds.

For decades, the search for alien life has been guided by a simple idea: find planets in the “habitable zone,” the region around a star where liquid water can remain on the surface. In our solar system, that familiar band stretches roughly from Earth’s orbit toward Mars.