Radio Beacons with a Minute-Long Rhythm: Who Lights Them Up
A lighthouse that blinks not every second but once every few minutes or even hours. That is exactly how long-period radio transients behave — cosmic sources discovered only recently.
Tides Steal Moons from Close-In Planets
The birth of a moon is a cosmic car crash. Two young planets collide, and a cloud of scorching debris swirls around the surviving world. From this disk, like clay on a potter's wheel, a satellite gradually takes shape. That's probably how our Moon came to be.
Planetary Collisions and Their Hydrogen Coat
In a single star system, two teams of planets orbit. Some follow neat paths, like figure skaters on an ice rink, avoiding collisions. Others crowd together, their trajectories cross, and sooner or later a cosmic accident occurs — a giant impact.
Cosmic Waltz: How a White Dwarf Became a Radio Beacon
In 2022, astronomers began discovering strange cosmic beacons — long-period radio transients. Unlike fast pulsars, discovered by Jocelyn Bell Burnell in 1967, these objects flared with periods of tens of minutes and hours.
The Swirling Dance of Neutron Stars
Two neutron stars whirl in their final dance. If their spin aligns with their orbital motion, the partners merge neatly, launching a narrow jet of superheated matter. If they spin in opposite directions, the dance breaks apart, scattering a thick shroud of debris.
How to Hear a Planet Near a Dead Star
The first exoplanet was discovered around an unusual cosmic lighthouse — a neutron star known as a pulsar. These ultra-dense remnants of dead stars spin at tremendous speeds and emit precise radio pulses.
Dust Rings at the Edge of a Distant System
A huge rotating pancake of gas and dust surrounds a young star. In such a "maternity ward" for planets, rings and gaps are often seen, as if an invisible plow had carved furrows. These are usually attributed to already-formed planets that clear paths with their gravity.
The Gravitational Orchestra Loses Its Rhythm
A figure skater glides across the ice, gradually moving toward the center. Their trajectory isn't a perfect spiral: sometimes they catch the rhythm of the music and add an extra turn, slightly changing their speed. That's roughly how a small black hole behaves when it falls into a supermassive one.
Planetary Orbits: Not Random, But Music
A guitar string only sounds at certain notes, when pressed at the frets. So it is with the gas-dust disk around a young star: it's shot through with standing waves, but only chosen oscillations survive. Where the wave crests, cosmic dust and hydrogen collect, and later exoplanets are born.
A Distant Planet's Magnetic Pulse
The star GJ 436 is a dim red dwarf, and orbiting it is a Neptune-sized planet on a nearly vertical, tilted orbit. Astronomers spent 18 years taking spectra of this star to track its spots and flares. Suddenly, a rhythm emerged in the data that matched neither the star's rotation nor its 8-year activity cycle. This rhythm exactly followed the planet's orbit.
Why Planets Fall Out of Rhythm
Young planetary systems resemble an orchestra that has just started rehearsing: all the musicians strive to play in the same rhythm.
Moons of Distant Planets: What's Keeping Us from Seeing Them
The light from a distant star is never steady. It shimmers like heat over hot asphalt. When astronomers pointed JWST at the star TOI 700, they saw this shimmer especially clearly: every 16 minutes, the brightness changed by a tiny fraction, just 46 parts per million.For comparison: if you placed a light bulb a kilometer away, this change would be…
How Orbits Reveal a Planet's Past
The Kepler telescope spent years watching thousands of stars, spotting planets by the tiny dips in starlight when a planet passes in front of its star. Such a passage, or transit, lets us measure the planet's size but not the shape of its path.
Orbiting Clocks Hunt for Invisible Fields
In August 2017, gravitational wave detectors caught a signal from the merger of two neutron stars — the ultra-dense remnants of exploded stars. At that very moment, life on Earth was business as usual: planes were landing, cars were driving, and navigators were plotting routes.
The Stumbling Dance of Two Planets Around TOI-4495
Two planets around the star TOI-4495 perform a stumbling dance: while the inner one completes two laps, the outer manages just one. But the rhythm is off — the inner planet speeds up and slows down, like a partner stumbling in her steps.
Using the transit method, watching as the planets briefly dim the star's light, astronomers weighed these worlds.
Deadly Resonance: How Stars Toss Out Planets
Two stars, drawing together in a cosmic dance, experience an extra wobble — a consequence of spacetime curvature (an effect predicted by Einstein). A planet orbiting them also wobbles. Sometimes the rhythms align: the gravitational tugs from the stars fall in step with the planet’s orbit, like hands pushing a swing.
Shadow or Mirage: Hunting a Moon Around a Scorching Jupiter
The hunt for exomoons — the search for satellites around planets of other stars — resembles watching shadows in a theater where the spotlight keeps fading and flaring. The planet Kepler-167e, a gas giant near a scorching star, was discovered by William Borucki and his team.
Noise as an X-ray: How Hidden Triplet Superconductivity Emerged at a Superconductor-Iron Interface
Run a current through a contact between a superconductor and a ferromagnet, and you will hear the whisper of the quantum world. In the lab at 0.3 K, that whisper turned into a roar: the shot noise—electrical noise due to the discreteness of charge—was a hundred times louder than theory allows for ordinary contacts.