“Artist’s impression of ZTF J0440+2325, a brown dwarf (right) and a red dwarf (left) that orbit each other every 86.65 minutes. The brown dwarf overflows onto its companion. And the stream of material strikes the surface. Of. The red dwarf, heating a large hot spot at the point of impact. Credit: Aaron Householder (MIT). (ScitechDaily, MIT Astronomers Catch a Star Slowly Eating Its Companion 300 Light-Years Away)
Before we go to thinking about white dwarfs. And their planetary systems. We must see the news. An. Interesting case. There, the red dwarf pulls matter from its brown dwarf companion. That causes intense heat in the red dwarf's atmosphere. That heat forms radio waves and X-rays. Maybe brown dwarfs can also steal matter from each other. When those material bridges impact other brown dwarfs. That can form radio bursts. We can see them. Coming from nowhere. Maybe brown dwarfs orbit some bright stars. When those bright stars, or maybe white dwarfs, steal their atmosphere. That can form extraordinary radio waves.
“The traces of sodium in the atmosphere of this white dwarf absorb the orange part of the spectrum, leaving behind a ghostly green glow."(Space.com, Astronomers discover the 1st ever green star, a cosmic zombie just in time for Halloween)
Astronomers discovered the first green star. It’s a white dwarf. A star that used up its fuel. Destroyed in a nova eruption. Then it turned into a white dwarf. That is the fate of the Sun when it uses up its hydrogen and helium. That star used all its fusion fuel. It can no longer produce energy. And gravity pulls it into a very dense object. That object is a white dwarf. If. The star is similar to the Sun. The WD J1330+6435. It is an almost typical white dwarf. But that star is green. And. That tells us that not all white dwarfs are white. Some of them are green, pink, or vivid blue. In. The case of WD J1330+6435. Sodium in its atmosphere makes that star look green.
The chemical environment determines white dwarf color. White dwarfs form in nova eruptions. When. A star uses all its fusion fuel. It. Blows its shell into space. That remnant forms an interplanetary nebula. And there is a possibility. That post-stellar planets can form in that remnant. There is a possibility. That the Hubble Space Telescope found the planet in the HS 0209+0832 system is a second-generation planet orbiting a white dwarf star. This means the planet formed after the star turned into a white dwarf. And that is one of the most interesting observations in the history of astronomy.
“Colour-accurate simulated images of white dwarfs. (Image credit: Mark Hollands/University of Warwick)(Space.com, Astronomers discover the 1st ever green star, a cosmic zombie just in time for Halloween)
There are predictions. And theories about the existence of such planets. But. The confirmation. Of. The existence of post-stellar planets is pending. The term post-stellar planet means that a planet forms from a planetary nebula around a white dwarf, neutron star, or black hole. The fact is that. All elements. In every planet, formed in dead stars. The question is: Could the planet form in the planetary nebula? That formed when a star erupted last time? And remained to orbit the star remnant.
The thing. That determines this possibility. It is the nebula’s density. And the nebula must not be too homogeneous. If. There are no denser points. gravitational dots, the planets cannot form. The model is that the destroyed planet’s cores pull that material around them. And form a new planet around them.
“This artist’s concept depicts a possible explanation for the unusual chemical abundances NASA’s Hubble Space Telescope detected in the HS 0209+0832 system: a second-generation planet orbiting a white dwarf star. Credit: NASA, ESA, Leah Hustak (STScI)”. (ScienceDaily, Hubble Space Telescope may have found a planet born after its star died)
A too-homogeneous nebula packs itself into one point. If the eruption is too strong, that nebula turns too thin. And of course. The eruption's symmetry plays a big role in that formation process. If. The eruption is like a giant flare. It can form a nebula. That is like a banner. The energy in that ionized gas can push plasma away and destroy the form. That forms a thin nebula. Elements like silicon can be found in that nebula.
When. A white dwarf is a middle-aged stellar remnant. Its gravity. Pulls particles into its shell. Those impacts form radiation. The wavelength of that radiation depends on those particles’ energy levels. And, of course. The element that impacts. The white dwarf is another determinant of radiation. Or its wavelength. The nebula. The white dwarfs can have regular stellar companions. The best-known case of that kind of binary system is Sirius.
The young blue star has the white dwarf companion Sirius B. So, stars can have companions formed long before them. Some bright stars have dim companions. Those companions can be brown dwarfs. They cannot affect Large stars' trajectories. That means. They cannot be seen using the methodology. Used. For exoplanet hunting. When a star in a binary star system is brighter. And. It steals matter from the dim component. A material bridge forms a hot spot in the star’s atmosphere. This means the dim component forms a brighter spot in the brighter star's atmosphere. So that thing is the opposite of the effect. The planet dims the star.
https://news.mit.edu/2026/astronomers-catch-star-slowly-snacking-on-brown-dwarf-1005
https://www.sciencedaily.com/releases/2026/10/261007042106.htm
https://scitechdaily.com/mit-astronomers-catch-a-star-slowly-eating-its-companion-300-light-years-away/
https://scitechdaily.com/nasa-hubble-cold-case-a-dead-star-may-have-given-birth-to-a-new-planet/
https://www.space.com/astronomy/stars/astronomers-discover-the-1st-ever-green-star-a-cosmic-zombie-just-in-time-for-halloween
https://en.wikipedia.org/wiki/Sirius





























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