Source: timesofindia
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Indian astronomers from the National Institute of Science Education and Research of Odisha have studied GG Tau A a rare triple-star system located 489 light-years from Earth.
GG Tau A is no ordinary star system. Its unique characteristics include:
Three stars orbiting each other in a gravitational dance. Rare among the known star systems in the universe.
A young system only 1 to 5 million years old making it ideal for studying the initial stages of planetary formation.
Surrounding these stars is a disk of gas and dust the building blocks for planet formation.
Using radio telescopes in Chile’s Atacama Desert scientists focused on the coldest regions of the disk.
Temperatures range between 12 to 16 Kelvin (-261 to -257°C) lower than the freezing point of carbon monoxide.
Icy molecules freeze into tiny dust particles which are the precursors to planetary building blocks. These particles clump together in super-cold conditions forming larger structures over time.
Cold temperatures allow gas and dust to stick together.
Warmer regions inhibit this process making planet formation more challenging.
This study highlights that cold, icy conditions are essential for planet formation especially in distant systems.
The three stars exert complex gravitational forces on the surrounding disk. These interactions disrupt the disk creating unique challenges for planet formation.
Unlike single-star systems the gas and dust in GG Tau A’s disk behave unpredictably. This makes the system a natural laboratory for understanding planet formation in multi-star environments.
Aspect |
Details |
Definition |
The process by which dust and gas in a protoplanetary disk around a star coalesce to form planets. |
Stages of Formation |
1. Nebular Collapse: Dust and gas collapse under gravity to form a protoplanetary disk. 2. Planetesimal Formation: Small particles stick together to form larger clumps (planetesimals). 3. Protoplanet Formation: Planetesimals merge into protoplanets through collisions. 4. Planetary Accretion: Protoplanets gather more material growing into fully formed planets. A protoplanet is a large planetary embryo that originated within a protoplanetary disk and has undergone internal melting to produce a differentiated interior. Protoplanets are thought to form out of kilometer-sized planetesimals that gravitationally perturb each other's orbits and collide, gradually coalescing into the dominant planets. |
Role of Temperature |
Cold regions enable gas and dust particles to stick together and grow. |
Key Factors Influencing |
Single vs. multi-star systems affect gravitational forces. Composition of gas and dust in the disk. Extremely low temperatures allow particles to freeze and stick together. Interactions in multi-star systems can disrupt or enhance formation. |
Sources:
PRACTICE QUESTION Q.Discuss the process of planet formation in protoplanetary disks and the role of temperature in this process. Provide examples from recent discoveries. (250 words) |
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