The Science of Life – From Earth to the Stars

what is dark energy — Type Ia supernova explosion in a distant galaxy — the observations that led to the discovery of dark energy and the accelerating universe

What Is Dark Energy? The Force Accelerating the Universe’s Expansion

In 1998, two independent teams of astronomers studying distant supernovae made a discovery that upended cosmology. They expected to find that the universe‘s expansion was slowing down, pulled back by the gravity of all the matter within it. Instead, they found the opposite: the expansion of the universe is accelerating. Something is pushing space apart faster and faster. That something is what we now call dark energy. What is dark energy? That question, unanswered since the discovery of cosmic acceleration in 1998, may be the most important open problem in cosmology. Dark energy is the name for whatever is causing the accelerating expansion. It makes up approximately 68% of the Read more

Artist impression of Proxima Centauri b, the nearest known exoplanet, orbiting the red dwarf star Proxima Centauri. Credit: ESO/M. Kornmesser

Proxima Centauri b: Our Nearest Known Exoplanet and What It Could Mean for Life

The nearest star to the Sun is Proxima Centauri, a red dwarf 4.24 light-years away in the constellation Centaurus. In 2016, astronomers announced that Proxima Centauri hosts a planet, Proxima Centauri b, orbiting squarely within the star’s habitable zone. No other confirmed exoplanet is closer to Earth. If any world beyond our solar system were to be visited or even contacted within any timeframe humans can meaningfully imagine, this is the most likely candidate. The discovery set off intense scientific debate that continues to this day. Does this planet have an atmosphere? Could it support liquid water? Does the violent activity of its host star sterilize its surface? And is Read more

A black hole slowly evaporating through Hawking radiation — particle pairs splitting at the event horizon

Hawking Radiation Explained: How Black Holes Slowly Evaporate

Black holes are defined by the impossibility of escape. Nothing that crosses the event horizon, the boundary of no return, can ever get out. That is the foundational property of a black hole, derived directly from general relativity. Yet in 1974, Stephen Hawking used quantum mechanics to show that black holes do emit radiation. They lose mass. They evaporate. And eventually, if left alone long enough, they disappear entirely. This result, Hawking radiation, is one of the most profound in all of theoretical physics. It connects general relativity, quantum field theory, thermodynamics, and information theory in ways that still generate active debate nearly fifty years later. The Vacuum Is Not Read more

Higgs boson particle physics visualization

The Higgs Boson Explained: The Particle That Gives Everything Mass

On July 4, 2012, physicists at CERN announced one of the most anticipated discoveries in the history of science. After nearly fifty years of searching, they had found the Higgs boson, a particle so fundamental to the workings of the universe that it had been called, somewhat controversially, the “God particle.” The announcement came from two independent detector teams at the Large Hadron Collider, both reporting a new particle consistent with the theoretical prediction. The Standard Model of particle physics was complete. But what is the Higgs boson, why does it matter, and why did it take nearly half a century to find? Why Particles Have Mass: The Higgs Field Read more

how black holes form — Artist illustration of a massive star collapsing in a supernova to form a stellar-mass black hole

How Black Holes Form: Stellar Collapse, Mergers, and the Early Universe

A black hole is not a thing in the ordinary sense; it is a region of spacetime where gravity has become so extreme that nothing, not even light, can escape once it crosses the event horizon. Understanding what a black hole is requires understanding how it forms. And the answer turns out to depend entirely on mass. Different masses produce black holes through different processes, on different timescales, in different corners of the universe. Here is how black holes form: through several distinct physical processes, each leaving a different signature on the black hole’s mass and environment. Stellar Collapse: The Main Factory The most common path to a black hole Read more

falsifiability — Portrait of Karl Popper, the Austrian-British philosopher who developed the principle of falsifiability as the criterion for scientific claims

Falsifiability Explained: How Karl Popper Defined the Boundary of Science

In 1919, Karl Popper noticed something that bothered him about several popular theories of the time. Freudian psychoanalysis, Adlerian psychology, and Marxist historical theory all shared a curious property: they could explain anything. Whatever happened, the theories could accommodate it. A patient improved, the theory explained it. A patient got worse, the theory explained that too. Any historical event could be reinterpreted as confirming the Marxist framework. The theories seemed powerful precisely because nothing could refute them. Popper contrasted this with Einstein’s general relativity, which made a very specific prediction: light would bend around the Sun by a precise amount during a solar eclipse. If the 1919 eclipse observations had Read more

europa vs enceladus — Europa's cracked ice surface photographed by NASA, showing reddish-brown linea believed to be briny water from the subsurface ocean

Europa vs Enceladus: Which Ocean Moon Is More Likely to Harbor Life?

Two moons in our solar system have confirmed liquid water oceans beneath their icy surfaces. Both are geologically active. Both have been touched by spacecraft. And both are now central to the question of whether life exists anywhere beyond Earth. The question of which ocean moon is the better candidate for life, Europa or Enceladus, is the defining astrobiology question of the coming decade. Europa orbits Jupiter, 628 million kilometers from the Sun. Enceladus orbits Saturn, 1.27 billion kilometers out. Despite their distance from each other and from the warmth of the Sun, both harbor more liquid water than Earth’s oceans. What separates them is not water. It is evidence. Read more

titan moon saturn — NASA Cassini spacecraft image of Titan, Saturn's largest moon, showing its thick orange nitrogen and methane atmosphere

Titan: Saturn’s Strange Moon and the Most Earthlike World in the Solar System

If you could stand on Titan and look up, you would see a thick orange haze blocking all but a faint glow from the distant Sun. The air pressure around you would be about 1.5 times that of Earth at sea level (comfortable, in a sense), but the temperature would be around −179°C (−290°F), cold enough to liquefy natural gas. Below your feet, the ground might be dusted with organic particles. In the distance, a river channel carved by liquid methane winds toward a vast methane lake. Titan (Saturn’s largest moon) is one of the most compelling destinations in the search for life beyond Earth. Titan is Saturn’s largest moon Read more