Skip to main content

TRAPPIST-1 There are 7 planets in the Solar System, out of which 5 are the size of Earth.



In 2017, on February 22, NASA announced a solar system whose star is a red dwarf star, which is orbited by Earth-sized planets, this solar system has seven Earth-sized planets, and this solar system  The star is known as TRAPPIST-1.  This solar system of TRAPPIST-1 is one of the unusual planetary systems discovered beyond our Sun, can there be life in any of the planets of TRAPPIST-1's star system, are any of its planets habitable.


TRAPPIST-1 is a supercool dwarf star located in the region of the constellation Aquarius, it is slightly larger than the planet Jupiter in our solar system and cooler than our Sun, and less than 10% its size, it is about 39.5 light-years away from the Sun. Five years after the first discovery, the planets of TRAPPIST-1 are still enigmatic, with researchers' studies showing that the solar system of TRAPPIST-1 may be almost twice as old as our solar system.


Sean Carey, manager of the Exoplanet Science Institute at NASA's Jet Propulsion Laboratory in Southern California, who was part of the team that helped find some of TRAPPIST-1's planets using data from the Spitzer Space Telescope, says Carey,  People have been able to ask the question, whether a planet around another star is habitable.  The researchers found that the planetary system of the TRAPPIST-1 star consists of seven terrestrial planets, five (b, c, e, f, g) that are similar in size to Earth, and two (d, h) of Mars (whose diameter  is about half that of Earth) and are between the size of Earth.


The Hubble Space Telescope added more information about TRAPPIST-1's potential to be habitable, of which at least three planets—d, e, and f—do not have the puffy, hydrogen-dominated atmospheres of gas giants,  However, Hubble does not have the power to determine whether the planets have potentially habitable atmospheres.


The Webb telescope, which was launched by NASA and ESA on December 2021, will investigate the planets of Webb TRAPPIST-1, the fourth planet from Webb's main target star, called TRAPPIST-1e. Scientists consider TRAPPIST-1e to be the habitable zone, because it lies in the Earth-like zone of life, also known as the Goldilocks zone, the Goldilocks orbital distance of a star where liquid water is found on a planet's surface,  just the right amount of heating to allow.


What makes a planet habitable, if anything, is its atmosphere, how important the atmosphere is for a planet, they can be understood from the atmosphere of the Earth. The researchers expect to get only a partial indication from Webb, especially in their initial observations, as to whether any atmospheres exist.


Lewis is part of the science team that will observe the sky in infrared light using the Webb telescope, says Lewis, who needs to watch TRAPPIST-1e's atmosphere as it falls into the Goldilocks perch in the habitable zone. Lewis goes on to say, that we expect, that we see carbon dioxide, a really strong feature, at wavelengths [detectable by the web]. Once we know where the little things that rise above the noise are, we can go back and see a lot more resolution in that area.


To try to deduce their possible composition, Lewis says, they should use computer models to construct possible planetary environments, as these may prove to be important options for understanding the TRAPPIST-1 planets. The great thing about the TRAPPIST system, says Lewis, is that it allows us to refine those models in any way they want, whether they'll just become barren reefs, or potentially habitable worlds.



Comments

Popular posts from this blog

NASA/ESA Hubble Space Telescope Reveals New Details of the Orion Nebula’s Star Formation.

  This NASA/ESA Hubble Space Telescope image captures the Orion Nebula (Messier 42, M42), the nearest star-forming region to Earth, located about 1,500 light-years away. A captivating new image captured by the NASA/ESA Hubble Space Telescope offers an extraordinary look into the Orion Nebula, the nearest massive star-forming region to Earth. Located just 1,500 light-years away, this nebula is visible to the naked eye below the three stars forming Orion's "belt." The region is home to hundreds of newborn stars, including two protostars featured in the image: HOPS 150 and HOPS 153. Named after the Herschel Orion Protostar Survey, conducted with ESA’s Herschel Space Observatory, the protostars HOPS 150 and HOPS 153 provide key insights into the early stages of star formation. HOPS 150, visible in the upper-right corner of the image, is a binary star system, with two young stars orbiting one another. These protostars are surrounded by small dusty disks, where material from th...

New Method Detects Small Asteroids in Main Belt, Offering Insight for Planetary Defense.

  An international team of physicists, led by MIT researchers, has developed a groundbreaking method to detect small asteroids, as small as 10 meters in diameter, within the main asteroid belt. These space rocks, ranging from the size of a bus to several stadiums wide, were previously undetectable using traditional methods. The team's discovery, detailed in a paper published in Nature, could significantly improve tracking of potential asteroid impactors, aiding planetary defense efforts. The main asteroid belt, located between Mars and Jupiter, is home to millions of asteroids, but until now, scientists could only detect objects roughly a kilometer in diameter. The new detection technique, which utilizes the "shift and stack" method, is able to identify much smaller asteroids, even those far from Earth, enabling more precise orbital tracking. This breakthrough is crucial for planetary defense, allowing scientists to spot near-Earth objects that may pose a threat in the fu...

XSPECT Payload Successfully Validates Performance through Cas A Observation.

  The XSPECT instrument captures a detailed spectrum of the supernova remnant Cassiopeia A (Cas A), encompassing both the Galactic Cosmic Ray (GCR) background and the Cosmic X-ray Background (CXB). The flux observed above 8 keV predominantly results from the combined contributions of CXB and GCR. The presented spectrum, depicted in the figure, is derived from a cumulative integration time of 20 ksec, collected across multiple orbits, providing valuable insights into the X-ray emissions associated with Cas A. XPoSat, India's inaugural X-ray polarimetric mission, has achieved a significant as the XSPECT instrument captures its initial observations from the Cassiopeia A (Cas A) supernova remnant. Launched on January 1, 2024, XPoSat is equipped with two co-aligned instruments, namely the POLarimeter Instrument in X-rays (POLIX) and X-ray SPECtroscopy and Timing (XSPECT). This mission is designed to unravel the mysteries of cosmic X-ray sources. While POLIX focuses on examining X-ray po...