![]() During these changes it will go through the planetary nebula phase, and white dwarf phase. What happens next depends on how massive the star is.Ī smaller star, like the Sun, will gradually cool down and stop glowing. All stars will expand, cool and change colour to become a red giant. The star then enters the final phases of its lifetime. ![]() Smaller stars use up fuel more slowly so will shine for several billion years.Įventually, the hydrogen which powers the nuclear reactions inside a star begins to run out. This means they may only last a few hundred thousand years. Very massive stars use up their fuel quickly. The exact lifetime of a star depends very much on its size. This stage is called the ' main sequence'. Astronomers hope to find even more of these lower energy transient events to help us understand the complex relationships between planets and their parent stars.Nuclear reactions at the centre (or core) of a star provides energy which makes it shine brightly. ![]() We still do not know the details of the system or how this planet came to be so unlucky. Needless to say, the interaction between the planet and the star over the course of its engulfment released an incredible amount of energy resulting in the red nova. ![]() However, the accretion disk itself would be capable of launching its own jets which could punch away from the star, expanding and nebula away from the system. Material from the destroyed planet slowly leaked and funneled into the star before it was all finally over. Before complete engulfment, the planet might have formed an accretion disk around the star itself. However, those jets were not powerful enough to escape from the gravitational influence of the star completely, and so that material rained back down.īut even though the planet reacquired some of its mass lost in the form of the jets, the planet lost it again due to the intense energies near the surface of the star. Complex flows of electricity and magnetism caused this plasma to launch a pair of jets away from the planet as it was orbiting the star. Instead it went through several violent phases as the planet was torn apart and the red nova flared.Īs the planet neared the star it heated up, with its outer layers turning into a plasma. The astronomer behind the study concluded based on theoretical calculations that however this planet ended up getting close to its star, it was not a simple matter of the planet slipping into the atmosphere of the star and calling it a day. The research is published on the arXiv preprint server. But in this case the star is on the main sequence, meaning that it is a normal middle-aged star. Previous cases of suspected star-planet interactions happen in very young systems, where planets are on chaotic trajectories, colliding into each other and occasionally diving headfirst into their stars. Several ILOT candidates have been closely examined with this scenario in mind, but astronomers have found it difficult to match up theoretical predictions of this scenario with the actual observational results.īut this new observation, known as ZTF SLRN-2020, may just fit the bill. But despite the rarity of the events, astronomers suspect that they occur very frequently throughout the universe.įor years astronomers have wondered if these red novas were caused by planets being engulfed by their parent stars. That makes it hard for us to capture them in observations. These are extremely rare events to observe, because they only produce a moderate amount of energy. The technical jargon term for these red nova events are "intermediate luminosity optical transits," or ILOTs.
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