Soulmate Gem
Photo by Johannes Plenio Pexels Logo Photo: Johannes Plenio

Who is the youngest planet?

The hot Jupiter exoplanet V830 Tau b, published in the same issue of the journal Nature as the discovery of K2-33b, is the youngest known exoplanet with an age of around 2 million years (around the time that humans evolved on Earth).

en.wikipedia.org - K2-33b - Wikipedia
What makes a man madly in love?
What makes a man madly in love?

Physical attraction, sexual compatibility, empathy, and emotional connection are key to making a man fall in love with a woman. Oct 3, 2022

Read More »
Which signs will find love in 2022?
Which signs will find love in 2022?

Lucky Zodiac Signs In Love 2022: Love Horoscope 2022 For 7 Lucky Signs Lucky Zodiac Signs In Love 2022. Is there love on your platter? ... Taurus....

Read More »

Young Super-Neptune orbiting K2-33

K2-33b (also known by its EPIC designation EPIC 205117205.01) is a very young super-Neptune exoplanet, orbiting the pre-main-sequence star K2-33. It was discovered by NASA's Kepler spacecraft on its "Second Light" mission. It is located about 456 light-years (140 parsecs) away from Earth in the constellation of Scorpius. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Among known exoplanets, K2-33b is considered extremely young − a mere 9.3 million years old. Only one other exoplanet is younger, with an age of 2 Myr (V830 Tau b).

Physical characteristics [ edit ]

Mass, radius, and temperature [ edit ]

K2-33b is a super-Neptune, an exoplanet that has a mass and radius larger than that of Neptune. It has an equilibrium temperature of 850 K (577 °C; 1,070 °F). It has a radius of 5.04 R Earth . While the exoplanet's mass hasn't been constrained yet, upper estimates place a mass of 3.6 M J .[1]

Atmosphere [ edit ]

By 2022, the atmosphere of K2-33b was found to be hazy, without any noticeable molecular bands in transmission spectrum. Given the planetary radius and temperature, atmosphere is likely to contain an abundant carbon monoxide and dense tholin haze.[4]

Host star [ edit ]

The planet orbits an (M-type) pre-main-sequence star named K2-33. The star has a mass of 0.54 M ☉ and a radius of 1.05 R ☉ . It has a surface temperature of 3540 K and is 9.3 million years old. In comparison, the Sun is 4.6 billion years old[5] and has a surface temperature of 5778 K.[6] It has about the same amount of metals as the Sun, with a metallicity ([Fe/H]) of 0. Its luminosity ( L ☉ ) is 15% that of the Sun.[2] The star's apparent magnitude, or how bright it appears from Earth's perspective, is 14.3. Therefore, it is too dim to be seen with the naked eye.

Orbit [ edit ]

Why do women's thighs get bigger with age?
Why do women's thighs get bigger with age?

The ratio of body fat to muscle increases, as muscle mass decreases. Due to the aging factor, weight is being added to our thighs and buttocks. Oct...

Read More »
What are the three loves of God?
What are the three loves of God?

There are three different words for love in Greek, and each word means something different in scripture. Eros is based on feelings and is me-...

Read More »

K2-33b orbits its host star with an orbital period of 5.424 days at a distance of 0.049 AU (compared to the distance of Mercury from the Sun, which is about 0.38 AU). The planet likely receives about 125 times as much sunlight that Earth does from the Sun.

Age and formation [ edit ]

Artist's impression of K2-33b transiting its extremely young parent star.

The planet is best known for its remarkably young age, which is estimated to be about 9.3 million years.[2] Given this age, the planetary system most likely formed back near the end of the Miocene epoch of the Earth's history. Observations made on the planet confirmed that it was in fact a fully formed exoplanet, not just a protoplanet that was still in the stages of developing. The mass and radius of the exoplanet further help constrain this statement.[2][1] K2-33b is the youngest confirmed transiting exoplanet. There are relatively few other exoplanets discovered to date with an age this young, all of which are non-transiting (with some that were detected around the hot A-type and B-type stars, such as HD 95086 and HIP 78530, however these could just be brown dwarfs due to their mass). The hot Jupiter exoplanet V830 Tau b, published in the same issue of the journal Nature as the discovery of K2-33b, is the youngest known exoplanet with an age of around 2 million years (around the time that humans evolved on Earth).[7] The discoveries of K2-33b and V830 Tau b are most notable for explaining how close-in planets form, an open question in the field of exoplanets since the discovery of the first exoplanet, 51 Pegasi b, in 1995. Given the young ages of these exoplanets, several theories of planetary migration can be ruled out because they take too long to form close-in planets. The most plausible formation scenario for K2-33b is that it formed further away from its star, then migrated inwards through the protoplanetary disk, although it remains a possibility that the planet formed in place.[2][1] Trevor David of Caltech in Pasadena stated on the discovery of the exoplanet "The question we are answering is: Did those planets take a long time to get into those hot orbits, or could they have been there from a very early stage? We are saying, at least in this one case, that they can indeed be there at a very early stage."[8] Understanding the young ages of such exoplanets may eventually help to lead scientists on how planetary formation works and provide some clues on the origin of the Solar System and other such planetary systems discovered.

Is PDA an autism profile?
Is PDA an autism profile?

The PDA Society, a U.K.-based nonprofit, describes PDA as “a profile on the autism spectrum.” And the U.K.'s National Autistic Society calls PDA a...

Read More »
What phrases disarm a narcissist?
What phrases disarm a narcissist?

The following are 16 key phrases to disarm a narcissist: 1. “ ... “I Can't Control How You Feel About Me” ... “I Hear What You're Saying” ... “I'm...

Read More »

Discovery [ edit ]

In 2014, NASA's Kepler spacecraft began its "Second Light" mission, after two of its reactor wheels had failed the previous year, ending the primary mission. From 23 August to 13 November 2014, the spacecraft collected data from the core of Upper Scorpius, which included K2-33.[2] The exoplanet was simultaneously discovered by two independent research groups, one led by astronomers from the California Institute of Technology[1] and the other led by astronomers from the University of Texas at Austin.[2] The star was studied on days in late January, February, and March 2016. The observations were made with the Immersion Grating Infrared Spectrometer (IGRINS) on the 2.7-m Harlan J. Smith Telescope at the McDonald Observatory.[2] After observing the respective transits, which for K2-33b occurred roughly every 5 days (its orbital period), it was eventually concluded that a planetary body was responsible for the periodic 5-day transits. The discovery was announced on 20 June 2016 in an announcement made by NASA.[8]

See also [ edit ]

en.wikipedia.org - K2-33b - Wikipedia
Who gets over a breakup faster?
Who gets over a breakup faster?

There's a reason for this, according to new data from Match's Singles in America survey: Guys just get over breakups faster. Match surveyed more...

Read More »
What are the signs of missing someone?
What are the signs of missing someone?

Signs That You're Missing Someone Being consumed with thoughts about that person. Experiencing a sense of longing. Eating more or less than you...

Read More »
Is being touch starved a thing?
Is being touch starved a thing?

Touch starvation can happen anytime a person doesn't get enough physical contact. It's often seen in children in orphanages and older adults in...

Read More »
Who is the king of the fire signs?
Who is the king of the fire signs?

Aries (astrology) Aries Constellation Aries Zodiac element Fire Zodiac quality Cardinal Sign ruler Mars 8 more rows

Read More »