Space

Extraterrestrial life is life that may exist beyond Earth, from simple microbes in a buried ocean to possible organisms on planets around other stars. Scientists do not start by assuming aliens are present. They look for measurable signs: chemistry, minerals, light patterns, environmental conditions, and repeated observations that are hard to explain without biology. What This Search Is Really About The search for life beyond… 

A telescope is an instrument that collects radiation from distant objects, brings that radiation to a focus, and turns it into something people can study: an image, a measurement, or a spectrum. In everyday astronomy, the word usually means an optical telescope that works with visible light, but modern observatories also study infrared, ultraviolet, radio waves, X-rays, and other parts of the electromagnetic spectrum. A… 

Cosmic inflation is the idea that the very early universe went through an extremely short phase of accelerated expansion. It did not describe galaxies flying through space like pieces of debris. It described space itself expanding so rapidly that tiny early differences could be stretched across vast cosmic distances. The Simple Version Inflation is used to explain why the universe looks so even in every… 

A red giant is an aging star whose outer layers have expanded after hydrogen fusion in the core has slowed or stopped. A red supergiant is the larger, brighter late-life version reached by many massive stars. The two names sound similar, but they do not mean the same thing: ordinary red giants usually come from low- or intermediate-mass stars, while red supergiants are tied to… 

A planetary atmosphere is the layer of gas held around a planet, moon, or small world by gravity. Some worlds keep thick air for billions of years. Others hold only a thin exosphere, where atoms barely collide before drifting away. The difference comes from a balance between gravity, temperature, gas chemistry, sunlight, solar wind, impacts, and the way a world’s interior releases or absorbs gases.… 

A supernova is the explosion of a star at the end of a major stage in its life. In a short burst of light, heat, particles, and expanding gas, a star can release more energy than it produced across much of its normal lifetime. Supernovae matter because they scatter elements into space, shape clouds of gas, leave behind neutron stars or black holes in many… 

A white dwarf is the hot, compact leftover core of a low- or medium-mass star after the star has used up the fuel in its center and shed its outer layers. It is not a normal shining star with steady core fusion. It is a stellar remnant: small in size, high in density, and slowly cooling for billions of years. Most stars in the Milky… 

Hubble’s Law says that distant galaxies tend to move away from us faster when they are farther away. It is one of the main observations behind the idea that the universe is expanding, not as an explosion into empty space, but as a stretching of space itself. The short form is simple: velocity is proportional to distance. The Basic Idea in Plain English Hubble’s Law,… 

The cosmic microwave background, often shortened to CMB, is the cooled remnant of the first light that could travel freely through the Universe. It is not light from a star, galaxy, or nebula. It is a faint microwave glow that fills space in every direction, carrying information from a time when the Universe was still very young.[Source-a] A Clear Starting Point The CMB is often… 

Space weather is the changing state of the space environment around Earth, driven mainly by the Sun. The two names people hear most are solar flares, which are bursts of radiation, and coronal mass ejections, or CMEs, which are expanding clouds of plasma and magnetic field. When the timing, direction, and magnetic setup line up, those solar events can disturb radio links, navigation signals, satellite…