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The vast distances between stars make interstellar travel one of humanity’s most daunting challenges. Even the Voyager spacecrafts, now in interstellar space, would take tens of thousands of years to reach the nearest star, Alpha Centauri. To put this into perspective, Alpha Centauri is 277,000 astronomical units (AU) away—over 7,000 times the distance from Earth to Pluto. At current spacecraft speeds, a journey to our stellar neighbor would take an unimaginable 70,000 years. However, new ideas like the Sunbeam Mission offer a promising path forward, proposing innovative propulsion techniques that could shorten this timeline to mere decades.

The Sunbeam Mission centers around relativistic electron beam propulsion, where high-energy electron beams, accelerated close to the speed of light, push a spacecraft forward. This approach eliminates the need for onboard fuel, reducing the spacecraft’s mass and enabling greater acceleration. A stationary satellite, or statite, positioned near the Sun, would generate these electron beams by converting solar energy into electricity. Using materials and technologies like those developed for NASA’s Parker Solar Probe and European Space Agency’s Solar Orbiter, the statite could endure the Sun’s intense heat while directing the beam over vast distances. This could propel a spacecraft to 10% of the speed of light, allowing it to reach Alpha Centauri in about 40 years.

While the concept is ambitious, its challenges—like generating and maintaining the beam, energy conversion, spacecraft navigation, material durability, and beam focus—are not insurmountable. Current technologies, such as the Large Hadron Collider, high-temperature solar converters, and advanced heat-resistant materials, provide a foundation for overcoming these hurdles. Innovations in adaptive optics and laser communication systems also offer insights into managing beam precision over interstellar distances, demonstrating how existing advancements could be adapted for this revolutionary mission.

Electron transport in bilayer graphene exhibits a pronounced dependence on edge states and a nonlocal transport mechanism, according to a study led by Professor Gil-Ho Lee and Ph.D. candidate Hyeon-Woo Jeong of POSTECH’s Department of Physics, in collaboration with Dr. Kenji Watanabe and Dr. Takashi Taniguchi at Japan’s National Institute for Materials Science (NIMS).

The findings are published in the journal Nano Letters.

Bilayer graphene, comprising two vertically stacked graphene layers, can exploit externally applied electric fields to modulate its electronic band gap—a property essential for electron transport. This distinctive feature has drawn considerable attention for its prospective role in “valleytronics,” an emerging paradigm for next-generation data processing.

Dust storms on Mars could one day pose dangers to human astronauts, damaging equipment and burying solar panels. New research gets closer to predicting when extreme weather might erupt on the Red Planet.

Today’s weather report on Mars: Windy with a chance of catastrophic dust storms blotting out the sky.

In a new study, planetary scientists at the University of Colorado Boulder have begun to unravel the factors that kick off major dust storms on Mars — weather events that sometimes engulf the entire planet in swirling grit. The team discovered that relatively warm and sunny days may help to trigger them.