1. Home
  2. / Science and Technology
  3. / The rocky planet BD+05 4868 Ab, located more than 140 light-years away, loses mass equivalent to Mount Everest with each orbit of 30.5 hours and creates a tail of mineral dust stretching millions of kilometers as it slowly disintegrates in space.
Reading time 5 min of reading Comments 0 comments

The rocky planet BD+05 4868 Ab, located more than 140 light-years away, loses mass equivalent to Mount Everest with each orbit of 30.5 hours and creates a tail of mineral dust stretching millions of kilometers as it slowly disintegrates in space.

Written by Débora Araújo
Published on 21/04/2026 at 17:31
Updated on 21/04/2026 at 17:32
Seja o primeiro a reagir!
Reagir ao artigo

BD+05 4868 Ab reveals a planet in self-destruction, evaporating under extreme heat and leaving a trail of debris, offering rare clues about the physical limits of planetary survival.

In 2025, researchers from the Massachusetts Institute of Technology (MIT) released a discovery that caught the attention of the international scientific community: a rocky planet identified as BD+05 4868 Ab is in an active process of disintegration, losing material with each orbit around its star. The discovery was based on data from the TESS (Transiting Exoplanet Survey Satellite), a NASA mission dedicated to identifying exoplanets.

Located more than 140 light-years from Earth, the planet exhibits a rare and extreme behavior. It orbits its star in just 30.5 hours, an extremely short period that places it under intense radiation and extreme heat. This proximity causes its surface to be continuously vaporized, resulting in a constant loss of mass.

According to MIT researchers, the planet may be losing material equivalent to the volume of Mount Everest with each complete orbit, a figure that helps to gauge the intensity of the process.

Extreme heat transforms rocks into vapor and initiates the destruction process

The planet’s proximity to its star subjects it to extremely high temperatures capable of vaporizing solid materials. In this environment, surface minerals do not remain stable. Instead, they undergo a continuous evaporation process, where rocks are heated until they turn into vapor, this material is released into space and the planet’s gravity cannot fully retain these elements.

Simulation reveals the dust tails in the z–y plane, with the star in the background highlighting the impressive height reached by the material released by the planet. Image: Marc Hon et al. / The Astrophysical Journal Letters (adapted by the editorial team)

This phenomenon creates a kind of temporary “mineral atmosphere,” which is soon dispersed by stellar radiation. Over time, this process results in the gradual loss of the planet’s mass.

Mineral dust tail extends for millions of kilometers

One of the most impressive aspects observed is the formation of a dust tail, similar to that of a comet. As the vaporized material escapes from the planet, it condenses into solid particles that are dragged by the radiation of the star, forming an elongated structure that can extend for millions of kilometers.

This tail not only evidences mass loss but also allows scientists to study the internal composition of the planet without needing to observe it directly. This is because the released material carries chemical information about the planet’s interior.

Mass loss on a scale comparable to Mount Everest impresses researchers

The estimated mass loss equivalent to Mount Everest per orbit is not just a visual comparison but an indication of the intensity of the process. Considering that Everest is about 8,848 meters high and has a gigantic volume of rock, this analogy helps illustrate how quickly the planet is being consumed.

Simulation shows the ‘unraveled’ dust tails in the z–ϕ plane, revealing how far the material spreads along the planet’s orbit. Image: Marc Hon et al. / The Astrophysical Journal Letters (adapted by the editorial team)

This level of loss indicates that the planet is in an advanced phase of destruction, potentially disappearing completely on a relatively short astronomical scale. Although this process takes thousands or millions of years, it is considered fast in cosmic terms.

Orbit of 30.5 hours exposes planet to continuous and extreme radiation

The orbital period of 30.5 hours places the planet extremely close to its star, which intensifies the disintegration process. Unlike Earth, which has a stable orbit and is relatively distant from the Sun, BD+05 4868 Ab is practically “stuck” to its star.

This proximity generates a continuous flow of energy that prevents any geological or atmospheric stability. The planet does not have enough time to cool down, keeping its surface in a constantly unstable state.

Discovery allows studying the interior of a planet without drilling

One of the most relevant scientific aspects of the discovery is the possibility of studying the internal composition of a rocky planet. Normally, this is extremely difficult, as it is not possible to directly access the interiors of exoplanets, and observations are limited to the surface and atmosphere.

However, in the case of BD+05 4868 Ab, the ejected material provides a unique opportunity. By analyzing the composition of the dust tail, scientists can infer which elements are present in the planet’s interior. This transforms the object into a natural laboratory for planetary studies.

Phenomenon is rare and reinforces extreme diversity of worlds in the universe

Planets in an active process of disintegration are considered rare, especially with such clear evidence as observed in this case. Most detected exoplanets exhibit relative stability, even under extreme conditions.

Dust tail in the x–y plane, with trajectories of grains from the Hill sphere and the region in cyan indicating the Parker wind. Image: Marc Hon et al. / The Astrophysical Journal Letters (adapted by the editorial team)

BD+05 4868 Ab, however, represents a final stage of planetary evolution, where destruction becomes visible on an observational scale. This type of object broadens the understanding of the different possible fates for planets.

TESS data was fundamental in identifying the anomalous behavior

The TESS mission, from NASA, was responsible for detecting variations in the light of the host star, indicating the presence of the planet. These variations did not follow a typical pattern, leading scientists to investigate more deeply.

The irregular shape of the transit signal was one of the first indications that the planet was surrounded by dispersed material. This type of signature is characteristic of objects with tails, such as comets, which helped confirm the disintegration hypothesis.

Process may lead to the complete disappearance of the planet

With the continuous loss of mass, the planet’s final fate tends to be its complete destruction. As material is removed, the planet’s gravity decreases, further facilitating the loss of new elements.

This effect creates an accelerated cycle of disintegration, in which the planet becomes increasingly vulnerable. Eventually, it may completely disappear, leaving only scattered debris around the star.

Discovery challenges traditional models of planetary stability

The existence of a planet in an active process of destruction poses challenges to current models of planetary formation and evolution. These models need to explain:

  • How the planet reached such a close orbit
  • How long it can survive
  • What mechanisms regulate mass loss

BD+05 4868 Ab provides real data that helps test and refine these theories.

Do you believe that there are many planets being destroyed right now in the universe? Leave your opinion in the comments.

Inscreva-se
Notificar de
guest
0 Comentários
Mais recente
Mais antigos Mais votado
Feedbacks
Visualizar todos comentários
Débora Araújo

Débora Araújo é redatora no Click Petróleo e Gás, com mais de dois anos de experiência em produção de conteúdo e mais de mil matérias publicadas sobre tecnologia, mercado de trabalho, geopolítica, indústria, construção, curiosidades e outros temas. Seu foco é produzir conteúdos acessíveis, bem apurados e de interesse coletivo. Sugestões de pauta, correções ou mensagens podem ser enviadas para contato.deboraaraujo.news@gmail.com

Share in apps
0
Adoraríamos sua opnião sobre esse assunto, comente!x