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Space Exploration

New Habitable Zone Planet Discovered in Unique Star System

By Jonathan Bala July 26, 2024

New Habitable Zone Planet Discovered in Unique Star System

A Neptune-like planet has been discovered in the habitable zone of a binary star system, thanks to the efforts of citizen scientists. This discovery sheds light on planetary formation and stability in multi-star systems.

Summary

A Neptune-like planet, TOI 4633 c, was discovered in a binary star system’s habitable zone.
Citizen scientists played a crucial role in detecting this planet using data from NASA’s Transiting Exoplanet Survey Satellite (TESS).
The newly found planet has an exceptionally long orbit of 272 days.
The system also possibly hosts another exoplanet and is orbited by a second star.
This discovery provides valuable insights into planetary formation and stability within multi-star systems.
The findings were published in The Astrophysical Journal on April 30, 2024.
Follow-up observations revealed more peculiarities about the system, including the potential for a second planet and a binary star system.
The study highlights the significant contributions of citizen scientists in identifying long-orbit exoplanets.

Discovery of TOI 4633 c

The discovery of TOI 4633 c marks a significant milestone in the field of astronomy, highlighting the importance of collaborative efforts between professional scientists and citizen scientists. The Neptune-like exoplanet was identified through the transit method, where the planet crosses in front of its host star, causing a temporary dimming of the star’s light.

The transit method is typically used to identify planets with tight orbits, as they frequently pass between Earth and their host star, blocking light more often. However, TOI 4633 c is unusual due to its long orbit of 272 days. This makes it one of the few long-orbit planets discovered using TESS data.

The discovery of a planet in the habitable zone of a binary star system provides valuable data for understanding planetary formation and stability in multi-star systems. According to Nora Eisner, the lead author of the study and a research fellow at the Flatiron Institute’s Center for Computational Astrophysics, “Finding planets in multi-star systems is crucial for our understanding of how you can make different planets out of the same material.”

Role of Citizen Scientists

Citizen scientists played an instrumental role in the discovery of TOI 4633 c. The planet was first identified by volunteers who sifted through data collected by NASA’s TESS. The Planet Hunters TESS program allows anyone with an internet connection to search for undiscovered planets in the TESS data.

Simon Bentzen, a Danish citizen scientist, expressed his excitement about the discovery: “Every time I spot a possible transit, I can feel my heart beat faster and my excitement rise extensively. I’m very happy that I helped find the new system. I hope that the new planets can help contribute to our understanding of planet formation and help answer other interesting planetary questions.”

New Habitable Zone Planet Discovered in Unique Star System — This infographic shows new discoveries. These are about a system with many stars and planets. Credit goes to Lucy Reading-Ikkanda and the Simons Foundation.

Advanced Observations and Follow-Up Studies

After the initial identification by citizen scientists, a follow-up study was conducted by Eisner and her team. This involved analyzing the star’s radial velocity to detect tiny wobbles caused by the gravitational tug of nearby companions.

The follow-up study revealed that what was initially thought to be a single star is actually a pair of binary stars. These stars are currently too close to be distinguished individually from Earth, but archival observations over the past 119 years confirmed the binary nature of the system.

The study also indicated the presence of a potential second planet with a 34-day orbit. The new exoplanet, TOI 4633 c, has the second-longest orbit of any planet discovered with TESS data and is one of only five with orbits longer than 100 days.

Implications for Future Research

The discovery of TOI 4633 c opens new avenues for research into planetary formation and stability in multi-star systems. The brightness of the host star and the long orbit of the planet make this system an ideal target for future exomoon detection campaigns.

Eisner suggests that TOI 4633 c may have satellites or moons, which could offer solid surfaces for life to take hold. “If this planet were to have a moon, that moon would likely have a solid surface, which could then be a great place to find water,” she explains.

Determining the exact layout of the stellar system will take at least 30 years, as the two stars need to move farther apart. Confirming whether the planets orbit the same star or different ones could significantly enhance our understanding of how such systems remain stable over time.

Conclusion

The discovery of TOI 4633 c in the habitable zone of a binary star system underscores the valuable contributions of citizen scientists to the field of astronomy. This finding provides crucial insights into planetary formation and stability in multi-star systems and highlights the potential for future discoveries in similar systems.

References

Eisner, N. L., Grunblatt, S. K., Barragán, O., et al. (2024). “Planet Hunters TESS. V. A Planetary System Around a Binary Star, Including a Mini-Neptune in the Habitable Zone.” The Astrophysical Journal. DOI: 10.3847/1538-3881/ad1d5c

Hashtags:

#ExoplanetDiscovery, #CitizenScience, #BinaryStarSystem, #TOI4633c, #PlanetHunters, #Astronomy, #TESS, #HabitableZone, #NeptuneLikePlanet, #ExomoonDetection

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Technology

Phoenix Planet: A New Discovery That Defies Atmospheric Loss Theories

By Jonathan Bala June 9, 2024

Phoenix Planet: A New Discovery That Defies Atmospheric Loss Theories

Key Takeaway

Phoenix, a newly discovered exoplanet, retains a thick atmosphere despite being close to a red giant star, challenging existing theories on planetary evolution and atmospheric retention. This discovery, led by researchers from Johns Hopkins University, provides fresh insights into how planets can defy expectations in extreme environments.

Summary

Discovery: Phoenix is a rare exoplanet that retains a thick atmosphere close to its red giant star.
Significance: Challenges existing theories about planetary evolution and atmospheric retention in harsh stellar environments.
Characteristics: Smaller, older, and hotter than expected; 6.2 times the size of Earth and 60 times less dense than the densest “hot Neptune.”
Research Techniques: Utilized NASA’s Transiting Exoplanet Survey Satellite and the W.M. Keck Observatory to filter and combine data for precise measurements.
Implications: Provides new insights into planetary system evolution, particularly for Earth’s future atmospheric changes.
Future Discoveries: The research team has identified a dozen potential candidates for similar studies.
Publication: Findings published in The Astronomical Journal on June 5, 2024.

An artist's concept shows TIC365102760 b, nicknamed Phoenix. This planet can survive intense radiation from a nearby red giant star. Credit: Roberto Molar Candanosa/Johns Hopkins University. — An artist’s concept shows TIC365102760 b, nicknamed Phoenix. This planet can survive intense radiation from a nearby red giant star. Credit: Roberto Molar Candanosa/Johns Hopkins University.

Introduction

In a groundbreaking discovery, astronomers have identified an exoplanet, named Phoenix, that defies conventional expectations of planetary evolution and atmospheric retention. This planet, orbiting a red giant star, should have been stripped of its atmosphere due to intense radiation, yet it maintains a thick, puffy atmosphere. This finding, published by Johns Hopkins University researchers, challenges existing theories and opens new avenues for understanding planetary behavior in extreme environments.

Characteristics of Phoenix

Phoenix, officially designated TIC365102760 b, belongs to the rare category of “hot Neptunes.” Despite being situated close to its host star, Phoenix has retained a substantial atmosphere. This discovery is particularly surprising given the planet’s characteristics:

Size and Mass: Phoenix is 6.2 times larger than Earth and exhibits significantly lower density, being 60 times less dense than the densest known hot Neptune.
Orbit and Proximity: The planet completes an orbit around its red giant star every 4.2 days, at a distance six times closer than Mercury is to the Sun.
Age and Temperature: Phoenix is notably older and hotter than anticipated for planets in such proximity to a red giant star.

Unusual Atmospheric Retention

“This planet isn’t evolving the way we thought it would,” said Sam Grunblatt, the lead researcher from Johns Hopkins University. “It appears to have a much bigger, less dense atmosphere than we expected for these systems.” This phenomenon challenges our understanding of how atmospheres can persist in harsh stellar environments where intense radiation is expected to strip them away.

Table 1: Characteristics of Phoenix

Characteristic	Detail
Size	6.2 times the size of Earth
Density	60 times less dense than the densest hot Neptune
Orbital Period	4.2 days
Proximity to Star	6 times closer than Mercury to the Sun
Age and Temperature	Older and hotter than expected

Research Techniques

The discovery of Phoenix was made possible through innovative research techniques. Grunblatt and his team utilized NASA’s Transiting Exoplanet Survey Satellite (TESS) and the W.M. Keck Observatory to obtain precise measurements. TESS detects low-density planets by observing the dimming of their host stars’ brightness as they pass in front. The team enhanced this data by filtering out unwanted light and combining it with measurements of the stars’ wobbles caused by orbiting planets, observed by the Keck Observatory.

Implications for Planetary Evolution

The persistence of Phoenix’s atmosphere, despite its proximity to a red giant star, has significant implications for our understanding of planetary evolution. The slow atmospheric stripping observed in Phoenix suggests that other factors may influence atmospheric retention. This insight is crucial for predicting the future of Earth’s atmosphere as our Sun evolves into a red giant.

“We don’t understand the late-stage evolution of planetary systems very well,” Grunblatt noted. “This is telling us that maybe Earth’s atmosphere won’t evolve exactly how we thought it would.”

Potential for Future Discoveries

Phoenix’s discovery highlights the potential for finding other unusual exoplanets. Puffy planets like Phoenix are rare, with scientists estimating that only about 1% of stars host such planets. Their smaller size makes them challenging to detect, but Grunblatt’s team has already identified a dozen potential candidates for further study using their refined techniques.

Conclusion

Phoenix’s discovery marks a significant milestone in astrophysics, challenging existing theories and providing new insights into planetary evolution. The planet’s ability to retain a thick atmosphere despite intense stellar radiation prompts a re-evaluation of our understanding of atmospheric loss and planetary decay in extreme environments. As researchers continue to uncover more about these rare puffy planets, we can expect to learn even more about the diverse and complex nature of solar systems.

Table 2: Future Research Directions

Research Area	Description
Atmospheric Retention	Investigate factors influencing atmospheric persistence in extreme environments.
Late-Stage Planetary Evolution	Study how planetary systems evolve as their host stars enter late stages of life.
Detection Techniques	Refine methods for detecting small, low-density exoplanets.
Comparative Planetology	Compare atmospheric characteristics across different types of exoplanets.

Reference

“TESS Giants Transiting Giants. IV. A Low-density Hot Neptune Orbiting a Red Giant Star” by Samuel K. Grunblatt et al., The Astronomical Journal, June 5, 2024. DOI: 10.3847/1538-3881/ad4149
Johns Hopkins University Press Release, June 8, 2024.

Hashtags

#Astronomy, #Astrophysics, #Exoplanets, #PhoenixPlanet, #JohnsHopkinsUniversity, #NASA, #TESS, #KeckObservatory, #PlanetaryScience, #RedGiantStar

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Space-Based Navigation

TESS Discovery: The First Rogue Planet Detected

By Jonathan Bala April 25, 2024

TESS Discovery: The First Rogue Planet Detected

Key Takeaway

TESS (Transiting Exoplanet Survey Satellite) has discovered its first rogue planet, a free-floating or unbound planet not orbiting any star, using the gravitational microlensing technique, marking an exciting step in unraveling the mysteries surrounding these strange alien worlds.

Summary

Over 5,000 planets have been found orbiting other star systems, but there is another category of planets called rogue planets or free-floating planets (FFPs) that travel through space without being gravitationally bound to any star.
Rogue planets are thought to have been ejected from their host star systems during formation or due to gravitational interactions, but their origin is still debated.
Detecting rogue planets is challenging due to their limited emission or reflection of electromagnetic radiation, but gravitational microlensing, where a planet passes in front of a star and distorts its light, can reveal their presence.
TESS, launched in 2018, scans large portions of the sky to monitor the brightness of thousands of stars, and its observations can detect light changes that may indicate the passage of a rogue planet.
A team of astronomers led by Michelle Kunimoto has developed algorithms to identify potential rogue planet candidates from TESS data.
The team recently published their findings in the Astrophysical Journal, reporting one rogue planet candidate event associated with the star TIC-107150013, about 3.2 parsecs away, with a light curve lasting 0.074 days ± 0.002 days, showing features expected of a rogue planet.
This marks the first rogue planet discovered by TESS and an exciting step toward unraveling the mysteries surrounding these strange alien worlds.
Simulations suggest that rogue planets may outnumber bound planets across the Galaxy, and their formation mechanisms are still being studied, with high-mass rogue planets potentially forming in isolation from gas collapse and low-mass ones likely ejected from star systems.

TESS Discovery The First Rogue Planet Detected — This is an image of NASA’s Transiting Exoplanet Survey Satellite.

TESS Discovers its First Wandering World

In the vast expanse of our galaxy, a remarkable discovery has been made – the first rogue planet, a free-floating celestial body unbound to any star, has been detected by the Transiting Exoplanet Survey Satellite (TESS). This amazing discovery is a big step forward in our journey to understand these mysterious wanderers of space.

Even though scientists have discovered more than 5,000 planets circling other stars, there’s another kind of planet out there called rogue planets, or free-floating planets (FFPs). Unlike the ones that orbit stars, these wanderers roam through space without being tied to any particular star. These mysterious nomads have puzzled scientists for a long time, and where they come from is a topic of heated debate among astronomers.

One prevailing theory suggests that rogue planets were once part of planetary systems but were violently ejected during the chaotic formation process or due to gravitational interactions with other bodies. However, their creation mechanisms are still not fully understood, and alternative explanations, such as the collapse of gas clouds, are being explored.

Detecting rogue planets poses a significant challenge due to their limited emission or reflection of electromagnetic radiation. Traditional observational methods prove ineffective in capturing these faint, solitary wanderers. However, a technique called gravitational microlensing offers a unique solution.

Gravitational microlensing relies on the principle that a rogue planet, passing in front of a distant star, distorts the star’s light through its gravitational field, resulting in a brief brightness change. This fleeting signal is the key to unveiling the presence of these elusive worlds.

Launched in 2018, TESS has been a game-changer in the field of exoplanet exploration. By scanning vast swaths of the sky and monitoring the brightness of tens of thousands of stars, TESS has the capability to detect the subtle light changes indicative of a rogue planet’s passage.

Led by astronomer Michelle Kunimoto, a team of researchers has developed sophisticated algorithms to sift through TESS’s vast trove of data, separating potential rogue planet candidates from other celestial phenomena that could mimic their signatures, such as asteroids, bound exoplanets, and stellar flares.

In a recent publication in the Astrophysical Journal, the team reported the detection of a rogue planet candidate associated with the star TIC-107150013, located approximately 3.2 parsecs (10.4 light-years) away. The observed light curve, lasting 0.074 days ± 0.002 days, exhibited features consistent with a rogue planet’s gravitational microlensing signature.

This remarkable discovery marks the first confirmed rogue planet detected by TESS, igniting a new era of exploration and understanding of these enigmatic celestial nomads.

While only a handful of rogue planets have been detected so far, simulations suggest that these free-floating worlds may be more abundant than initially thought. Some models even predict that rogue planets could outnumber bound planets across the entire galaxy.

As our understanding of rogue planet formation mechanisms evolves, researchers hypothesize that high-mass rogue planets may have formed in isolation from the collapse of gas clouds, while low-mass counterparts were likely ejected from their parent star systems.

The discovery of TESS’s first rogue planet marks a significant milestone in our exploration of the cosmos, but it also raises captivating questions about the nature and origins of these enigmatic wanderers. As we learn more about rogue planets, we get closer to understanding how planets form. We also learn more about the complicated forces that shape our constantly growing universe.

HASHTAGS:

#RoguePlanets, #FreeFloatingPlanets, #TESS, #ExoplanetDiscovery, #GravitationalMicrolensing, #CosmicMysteries, #PlanetaryFormation, #SpaceExploration, #AstronomicalBreakthroughs, #GalacticAbundance #TESS Discovery

Source:

arXiv: “The Formation of the First Galaxies”: This arXiv preprint discusses the formation of the first galaxies, providing valuable insights into early cosmic evolution.

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