K2-33b

Coordinates: Sky map 16h 10m 14.74s, −19° 19′ 09.4″
Source: Wikipedia, the free encyclopedia.
K2-33b
K2 (Kepler) mission
Discovery date21 June 2016
Transit
Orbital characteristics
0.0409 +0.0021
−0.0023[3] AU
Eccentricity0.0[2]
5.424865+0.000035
−0.000031[2] d
Inclination89.1 +0.6
−1.1[2]
StarK2-33
Physical characteristics
Mean radius
5.04 +0.34
−0.37[2] R🜨
Mass<3.7 MJ
Temperature850 K (577 °C; 1,070 °F)

K2-33b (also known by its EPIC designation EPIC 205117205.01) is a very young

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

Mass, radius, and temperature

K2-33b is a

equilibrium temperature of 850 K (577 °C; 1,070 °F). It has a radius of 5.04 R🜨. While the exoplanet's mass hasn't been constrained yet, upper estimates place a mass of 3.6 MJ.[1]

Atmosphere

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

Main article: K2-33

The planet orbits an (

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

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

sunlight
that Earth does from the Sun.

Age and formation

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

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.

Discovery

In 2014,

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

  • V830 Tau b

References

  1. ^
    S2CID 4408972
    .
  2. ^
    doi:10.3847/0004-6256/152/3/61
    .
  3. ^ "K2-33b CONFIRMED PLANET OVERVIEW PAGE". NASA Exoplanet Archive. Retrieved 2016-07-06.
  4. S2CID 253523210
  5. ^ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
  6. ^ Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
  7. S2CID 1046761
    .
  8. ^
    National Aeronautics and Space Administration
    . 20 June 2016. Retrieved 1 September 2016.

External links
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