A recent study conducted by an international team of astronomers has revealed an intriguing phenomenon among twin stars. It is estimated that approximately one in every 12 twin stars exhibits signs of “ingesting” planets in their vicinity. These findings have challenged the previous assumption that twin stars have identical compositions.
The research team, led by astronomers from the All Sky Astrophysics in 3 Dimensions (ASTRO 3D) research center, employed three massive telescopes to observe 91 pairs of twin stars. Surprisingly, the team discovered that around eight percent of these twin stars displayed chemical differences, indicating the presence of planets or planetary material being “devoured” by one of the stars.
Dr. Fan Liu, a lead author of the study from Monash University in Australia, explained, “We looked at twin stars traveling together. They are born of the same molecular clouds and so should be identical. Thanks to this very high precision analysis, we can see chemical differences between the twins. This provides very strong evidence that one of the stars has swallowed planets or planetary material and changed its composition.”
While it is uncertain whether the stars are consuming planets whole or engulfing protoplanetary material, Dr. Liu suggests that both scenarios are possible. The study’s findings will have significant implications for understanding the long-term evolution of planetary systems, challenging the previous belief that such events were unlikely.
Associate Professor Yuan-Sen Ting, a co-author and an ASTRO 3D researcher, stated, “Astronomers used to believe that these kinds of events were not possible. But from the observations in our study, we can see that, while the occurrence is not high, it is actually possible. This opens a new window for planet evolution theorists to study.”
The study, which forms part of the Complete Census of Co-moving Pairs of Objects (C3PO) initiative, contributes to our understanding of the Chemical Evolution of the Universe. By shedding light on the distribution of chemical elements and their journey, including being consumed by stars, these findings pave the way for further exploration and provide novel insights into planetary evolution.
FAQ about Twin Stars and Planet Ingestion:
1. What did the recent study by astronomers reveal about twin stars?
The study found that approximately one in every 12 twin stars exhibits signs of “ingesting” planets in their vicinity. This challenges the previous assumption that twin stars have identical compositions.
2. How did the research team conduct their study?
The research team employed three massive telescopes to observe 91 pairs of twin stars.
3. What percentage of the observed twin stars displayed chemical differences?
Around eight percent of the observed twin stars showed chemical differences, indicating the presence of planets or planetary material being “devoured” by one of the stars.
4. Why is this significant?
The presence of chemical differences in twin stars suggests that one of the stars has swallowed planets or planetary material, which challenges the previous belief that such events were unlikely. This has implications for understanding the long-term evolution of planetary systems.
5. How did the study contribute to our understanding of the universe?
The study, part of the Complete Census of Co-moving Pairs of Objects (C3PO) initiative, sheds light on the distribution of chemical elements and their journey, including being consumed by stars. This contributes to our understanding of the Chemical Evolution of the Universe.
Definitions:
– Twin stars: Two stars that are born of the same molecular clouds and travel together.
– Ingesting: The process of a star consuming planets or planetary material.
– Chemical differences: Variations in the composition of elements present in the stars.
– Protoplanetary material: Material that forms planets in the early stages of planetary system formation.
Suggested Related Links:
ASTRO 3D Research Center
Monash University – Earth Atmosphere and Environment
The source of the article is from the blog macnifico.pt