Kepler 1652b Planet: Size, Mass, Gravity, Surface Temperature, Oxygen, Habitable, Atmosphere, Distance, Facts

Kepler 1652 b Planet

Embark on a cosmic journey as we delve into the enigmatic world of Kepler-1652 b, a super Earth exoplanet orbiting an M-type star.

Kepler 1652 b Size Compared to Earth in Percentage

The size of Kepler 1652 b is given as 1.60 R🜨 (radius). To express this in percentage compared to Earth, we can use the formula: $(\text{Radius of Kepler 1652 b}\mathrm{/}\text{Radius of Earth})\times 100$. Plugging in the values, we get $(1.60\mathrm{/}1.49)\times 100=\mathbf{\text{107.38\%}}$. Therefore, Kepler 1652 b is approximately 107.38% of Earth's size.

Kepler 1652 b Mass Compared to Earth in Percentage

The mass of Kepler 1652 b is provided as 3.19 Earths. To express this in percentage compared to Earth, we use the formula: $(\text{Mass of Kepler 1652 b}\mathrm{/}\text{Mass of Earth})\times 100$. Plugging in the values, we get $(3.19\mathrm{/}1)\times 100=\mathbf{\text{319\%}}$. Therefore, Kepler 1652 b has a mass approximately 319% of Earth's mass.

Kepler 1652 b Surface Gravity Compared to Earth

The surface gravity of a planet is determined by its mass and radius. Unfortunately, the radius of Kepler 1652 b is provided without the exact Earth radius value, making it challenging to precisely calculate its surface gravity compared to Earth.

Surface Temperature of Kepler 1652 b

The equilibrium temperature of Kepler 1652 b is 268 K (−5 °C; 23 °F). This temperature is similar to Earth's equilibrium temperature of 255 K (−18 °C; −1 °F).

Does Kepler 1652 b Have Oxygen

The information provided does not explicitly mention the presence or absence of oxygen in the atmosphere of Kepler 1652 b.

Is Kepler 1652 b Habitable

While Kepler 1652 b is located within the habitable zone of its star, habitability depends on various factors such as composition, atmosphere, and radiation. The planet's temperature is similar to Earth's, but its increased radius decreases its chances of habitability.

Kepler 1652 b Atmosphere Composition

The provided information does not specify the composition of the atmosphere of Kepler 1652 b. Details about the presence of gases, including oxygen, are not available.

Kepler 1652 b Distance from Earth in Light Years

Kepler 1652 b is situated approximately 822 light years away from Earth in the Cygnus constellation.

10 Interesting Fun Facts About Kepler 1652 b

1. Discovery: Discovered by NASA's Kepler spacecraft, Kepler 1652 b was first announced as a candidate in 2013 and validated in 2017.
2. Location: Orbits the red dwarf star Kepler-1652 in the Cygnus constellation, approximately 822 light years away.
3. Classification: Designated as a super-Earth with 160% Earth's radius, placing it within the transition range between rocky super-Earths and gaseous Mini-Neptunes.
4. Orbital Characteristics: Completes an orbit around its star in 38.1 days, with a semi-major axis of 0.1654 AU.
5. Temperature: Maintains an equilibrium temperature of 268 K (−5 °C; 23 °F), comparable to Earth's.
6. Host Star: Orbits the red dwarf star Kepler-1652, which is 0.404 times the mass and 0.382 times the radius of the Sun.
7. Habitability Factors: While within the habitable zone, its increased radius reduces chances of habitability. It receives about 81% of the sunlight Earth does.
8. Potential Eyeball Planet: Classified as an eyeball planet candidate due to its potential tidal locking to its host star.
9. Atmospheric Challenges: The high radius increases the likelihood of thick oceans or ice giant characteristics, affecting the development of life.
10. Distance and Age: Located 822 light years away, Kepler-1652 has an age of 3.2 billion years, making it much older than Earth.

Characteristics

Mass, Radius, and Temperature

Kepler-1652 b, discovered by NASA's Kepler spacecraft, boasts a mass equivalent to 3.19 Earths. Its intriguing radius of 1.60 R🜨 places it in the super-Earth category, suggesting a possible small ice giant or ocean planet. With an equilibrium temperature of 268 K, this exoplanet shares similarities with Earth in terms of temperature.

Orbit

This super-Earth completes one orbit around its M-type star, Kepler-1652, in just 38.1 days, highlighting its relatively short orbital period. Despite its proximity to the star, Kepler-1652 b maintains a temperate environment, thanks to the star's smaller size compared to the Sun.

Host Star

Orbiting the red dwarf star Kepler-1652, this exoplanet experiences the unique characteristics of its host. The star, with 0.404 times the mass and 0.382 times the radius of the Sun, presents intriguing conditions for Kepler-1652 b. Understanding the star's features enhances our comprehension of the exoplanet's habitability.

Habitability

Factors Influencing Habitability

Examining the intricate factors influencing Kepler-1652 b's potential habitability, from its position in the habitable zone to the nuances of its atmosphere.

Red Dwarf Flares and Habitability

Decoding the impact of red dwarf flares on Kepler-1652 b's habitability, exploring the delicate balance required for sustaining life beyond our solar system.

Discovery

Kepler Spacecraft's Contribution

Unveiling the pivotal role of the Kepler spacecraft in confirming Kepler-1652 b's existence, marking a milestone in exoplanetary exploration.

Orbital Characteristics

Analyzing the detailed orbital characteristics that define Kepler-1652 b's cosmic journey around its host star.

Conclusion

In the vast expanse of the cosmos, Kepler-1652 b stands as a testament to the wonders of our universe. Join us as we unravel the mysteries surrounding this super Earth, pondering the potential for life beyond the familiar realms of our solar system.