Our Milky Way, a vast spiral housing hundreds of billions of stars, is much more than a simple collection of suns and planets. It is a cosmic laboratory where the laws of physics are pushed to the extreme, giving rise to objects so strange that they sometimes defy physics. From stellar corpses that come back to life to worlds made of pure diamond, the Milky Way hides phenomena whose strangeness borders on the fantastic.
Through these five extraordinary objects, the entire cosmic cycle of matter is revealed: genesis, violent end, transmutation of matter, and recycling.
The term "zombie star" dramatically refers to a type of star that seems to come back to life after its theoretical death. These are usually neutron stars or white dwarfs, the ultra-dense remnants of stars like our Sun. The object is dynamically dead (end of nuclear fusion), but energetically reactivated by accretion or magnetic fields.
Their spectacular resurrection occurs in a binary system. If the white dwarf is close enough to a companion star, its intense gravity can "steal" matter from it. When this accumulated matter on its surface reaches a critical mass (about 1.4 solar masses), a cataclysmic nuclear fusion reaction is triggered. This is a neutron star, or even a nova where the "dead" star suddenly shines with prodigious intensity, sometimes visible to the naked eye from Earth, before returning to calm. This explosive cycle can even repeat.
Imagine a world whose crust and mantle are not made of silicate rocks like on Earth, but of pure diamond. The existence of these diamond planets is no longer science fiction.
They form from the remains of massive carbon-rich stars. When certain intermediate-mass stars evolve, they convert helium into carbon in their cores, but never reach the temperatures needed to fuse this carbon into oxygen. By expelling their outer layers, they enrich the interstellar medium with carbon, but not with oxygen. Planets that form from this material can therefore be exceptionally rich in carbon and poor in oxygen. After a cataclysm, extreme pressures and temperatures can crystallize the carbon into diamond. Exoplanets like 55 Cancri e are suspected to be largely composed of carbon in the form of diamond and graphite, around an iron core. Such a planet, with a radius twice that of Earth, could contain several times the Earth's mass in diamond.
Unlike all the planets we know, rogue planets (or interstellar planets) do not orbit any star. They wander alone in the black and cold immensity of interstellar space.
They can have two origins: either they formed alone, like failed stars too low in mass to ignite fusion and become brown dwarfs, or they were violently ejected from their natal planetary system by gravitational interactions. Astronomers estimate that they could be extremely numerous, perhaps even outnumbering the stars in the galaxy.
Current planetary formation models suggest that the protoplanetary disk of the young Sun gave rise to a hundred major planetary embryos competing in the inner and outer solar system. Some as massive as Mars or Mercury formed and coexisted unstably. The giant collisions that shaped our system, such as the one that created the Moon, testify to this violent period when the number of "candidates" for planet status was at least ten times greater than the final result.
Magnetars are a type of neutron star, whose hyper-dense remnant (a teaspoon of matter weighs billions of tons) comes from a massive star that exploded as a supernova. Magnetars possess a magnetic field of unimaginable power, billions of billions (1015) times stronger than Earth's.
In neutron stars, the layer of nuclear matter is so compact that it behaves like a solid of extraordinary rigidity. The magnetic field is so intense that it causes "starquakes" (star tremors analogous to earthquakes). These quakes release colossal bursts of gamma and X-rays, visible across the galaxy.
A magnetar at the distance of the Moon would make Earth uninhabitable in minutes, without even exploding. A gamma-ray burst would turn the event into an instant global extinction.
The exoplanet WASP-12b is a hot Jupiter, a gas giant orbiting so close to its star that its surface temperature exceeds 2500°C. WASP-12b is one of the darkest planets ever discovered.
It reflects less than 6% of the light it receives, making it exceptionally dark for a planet, darker than asphalt and close to the reflectivity of coal. This property contrasts sharply with that of Jupiter, which reflects more than 50% of sunlight. Scientists attribute this darkness to an atmosphere rich in titanium and vanadium hydroxides, chemical compounds that absorb almost all visible light. The extreme heat (over 1,000°C) also prevents the condensation of reflective clouds. What we observe from Earth is not the reflection of the star, but the faint intrinsic glow of its superheated atmosphere.
Note: WASP-12b in brief
Discovered in 2008, WASP-12b is a hot Jupiter orbiting so close to its star that it completes a revolution in 26 hours. Its albedo of less than 0.06 makes it one of the darkest known planets. Its shape is deformed by tidal forces and its atmosphere is actively evaporating under intense stellar radiation.
| Object | Type / Category | Main Feature | Known Example / Location |
|---|---|---|---|
| Zombie Star | White dwarf in a binary system accreting matter | Repeated thermonuclear explosions (novae) after its "death" | RS Ophiuchi, T Coronae Borealis (recurrent) |
| Diamond Planet | Carbon-rich terrestrial exoplanet | Dominant composition of diamond and graphite | 55 Cancri e (at ~41 light-years) |
| Rogue Planet | Interstellar planet or low-mass brown dwarf | Does not orbit any star, wanders in space | CFBDSIR 2149-0403 (potential, at ~100 light-years) |
| Magnetar | Neutron star with hyper-powerful magnetic field | Magnetic field ~1015 times stronger than Earth's | SGR 1806-20 (in the constellation Sagittarius) |
| Black Exoplanet | Ultra-hot Jupiter | Extremely low albedo (<6%), absorbs almost all light | WASP-12b (at ~1410 light-years) |
Source: Data compiled from NASA/ESA archives, publications in the Astrophysical Journal, and observations from the Hubble, Spitzer, TESS, and James Webb space telescopes.