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Space Astro
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Info for exoplanet "Naruhya Ba"
Scientific (actual) data |
Planet | K2-55 b |
Planet status | Confirmed |
Planet mass | 0.138 |
Radius | 0.341 |
Orbital period | 2.84926 |
Semi major axis | 0.03486 |
Orbit eccentricity | 0.124 |
Inclination | 88 |
Discovered | 2016 |
Updated | 2021-02-05 |
Omega | 195 |
Tconj | 2456980 |
Tzero tr | 2456980 |
Impact parameter | 0.37 |
K | 25.8 |
Temperature (kelvin) | 900 |
Publication | Published in a refereed paper |
Detection type | Primary Transit |
Mass detection type | Radial Velocity |
Radius detection type | Primary Transit |
Alternate names | EPIC 205924614.01 |
Star name | K2-55 |
Right ascension | 333.75° |
Declination | -17.25° |
Mag v | 13.6 |
Mag j | 11.23 |
Mag h | 10.615 |
Star distance | 160.26 |
Star metallicity | 0.376 |
Star mass | 0.7 |
Star radius | 0.63 |
Star temperature | 4456 |
Star alternate names | 2MASS J22150046-1715025, EPIC 205924614, WISE J221500.44-171502.7 |
Wikipedia article | K2-55 b |
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Fictional info (?) |
Suggested name | Naruhya Ba |
Planet type | Small hot gas planet |
Naruhya Ba's atmosphere is similar to Pimya Gedo's in its primary composition of xenon and ammonium hydrosulfide (NH4SH), but it contains more "ices" such as water, ammonia, and methane, along with traces of other hydrocarbons. The planet is named after the deity Naruhya Ba, the messenger of destruction.
As one of the most noticeable objects in the sky, Naruhya Ba has been a major fixture in native folklore for as long as records have existed.
It was the one of the first exoplanets visited by a spacecraft, and one of the first to be successfully landed on. Naruhya Ba's thick clouds make observation of its surface challenging in ultraviolet light, and the first detailed maps did not emerge until the arrival of the Magellan orbiter 52 years ago.
The rotational period and seasonal cycles of Naruhya Ba are likewise similar to those of Earth, as is the tilt that produces the seasons.
The two polar ice caps appear to be made largely of dust.
Its apparent magnitude reaches -3, which is surpassed only by Pimya Gedo, Hochu Myo, and K2-55.
Wind speeds can reach 144 metres per second. |
Atmosphere | Xenon | 65% |
Ammonium hydrosulfide (NH4SH) | 25% |
Argon | 6.8% |
2H2O | 2.9% |
Nitrogen | 0% |
Atmospheric pressure | 12 bar |
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Moon | Zatsuga Yamyurya | Large potato shaped crater-filled moon |
Sutsu Nyokya | Large irregular oceanic planetoid |
Kema Shisu'myo | Large irregular rocky moon |
Hato-shi | Very small round gaseous moon |
Kebyo Gehyu Sa | Medium-sized slightly egg-shaped ice moon |
Putae | Large almost round rocky moon |
Kenta-ijoma Hyo | Very small potato shaped ice comet |
Jasha-rosohyo | Very small almost round ice asteroid |
Kasha-gu | Huge slightly egg-shaped crater-filled comet |
Zana Chura | Large almost round oceanic asteroid |
Tohe Guchu-nyo | Small potato shaped ice moon |
Chiryo | Medium-sized almost round oceanic asteroid |
Rochuge-gyo | Large slightly egg-shaped oceanic planetoid |
Zuehyo | Medium-sized round rocky asteroid |
Nyusu Da | Small slightly egg-shaped ice moon |
Himasashu Pya | Medium-sized slightly egg-shaped ice moon |
Sojogya-wachu | Medium-sized round crater-filled moon |
Robe | Very small potato shaped gaseous planetoid |
Payonu Nkyu | Medium-sized round gaseous moon |
Google search for Naruhya ba |
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Website by Joachim Michaelis
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