Tidal Swings of an Eccentric Jupiter
Every 165 days, the giant planet dives toward its star, nearly grazing its fiery corona, then flies off into the icy void. This is TIC 241249530 b — an exoplanet with a record eccentricity of 0,94.
A Stellar Visitor Stirred Up the Comet Cloud
The giant cloud of icy chunks on the outskirts of the Solar System, the Oort cloud, resembles a transparent bubble stretched to a light-year across. Usually, these chunks hang quietly in their distant corners, but sometimes something disturbs them.
Most often, it's the tidal influence of our Galaxy.
The Magnetic Roots of the Solar Wind
The crown of a huge tree sways in the wind, but the roots and trunk are hidden underground. On the Sun, magnetic fields play the role of such invisible roots. They emerge from the depths, thread through the entire atmosphere, and govern the motion of the hot gas — plasma.
Forty Years of Tokamak Defiance, and the Breakthrough
In a pot of boiling soup, churning currents carry heat to the walls, and the soup cools. In a tokamak, a huge magnetic bottle for plasma, the same thing happens: turbulent eddies carry energy outward, hindering the ignition of a fusion reaction. But sometimes the plasma seems to find a way to calm itself.
How the Milky Way's Wind Tears Apart Clouds
A hair dryer aimed at a block of ice strips vapor and droplets from its surface, and the ice slowly melts. The wind from the center of our Galaxy works in much the same way: it picks up cold gas clouds and carries them away, heating and shredding them along the way.
Astronomers decided to systematically search this flow for molecules, the coldest and densest form of gas, for the first time.
Rooms of the Winter Sky: How the Atmosphere Chooses the Weather
In winter, air over the Northern Hemisphere does not move haphazardly; it spends days at a time in the same pattern before rearranging itself. These patterns are like rooms in a maze: the system enters, lingers, then finds a door to another room. Each room has its own weather: somewhere over Europe it is warm and humid, while over Siberia it is frosty and clear.
A Hurricane Thermometer: How One Metric Can Predict Their Numbers
Over warm ocean waters, air rises, spins, and turns into a giant vortex that carries winds faster than a race car. For such a vortex to form, several conditions must align: rotation, heat, moisture, and calm winds aloft. Previously, meteorologists combined these conditions into complex indices, like a kitchen recipe with a dozen ingredients.
How Ripples on Water Steer the Planet's Winds
The planet's winds are not free-flowing currents but rather obedient jets that can be nudged from an unexpected direction. The ocean surface, covered with waves, acts like a tuning knob: change its roughness, and giant air rivers shift by hundreds of kilometers.
The Salt Chronicle of the Messinian Crisis
A rock chronicle where each layer is a page, and spectral analysis reads the rhythm of the lines. In the Realmonte salt mine in Sicily, geologists measured the thickness of 120 three-part cycles: a millimeter-scale clay parting, a thin anhydrite or polyhalite layer, and then a decimeter-scale halite bed.
Hurricane Energy Follows a Power Law
A forest fire has no "typical" size: a small grass burn and a firestorm covering thousands of hectares are part of the same phenomenon. The same goes for tropical cyclones: the energy they release over their lifetime does not cluster around some average value. Instead, it follows a power law, and this rule holds across all of Earth's oceans.