|
|
Space Astro
|
Info for exoplanet "Ekyuge Kyo"
Scientific (actual) data |
Planet | Kepler-647 b |
Planet status | Confirmed |
Radius | 0.104 |
Orbital period | 16.2255 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454980 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J18590919+4435300 b, K00691.02, KIC 8480285 b, KOI-691 b, KOI-691.02, WISE J185909.19+443529.8 b |
Star name | Kepler-647 |
Right ascension | 284.79° |
Declination | 44.59° |
Mag j | 12.898 |
Mag h | 12.585 |
Mag k | 12.611 |
Star distance | 789 |
Star metallicity | -0.14 |
Star mass | 1.03 |
Star radius | 1.07 |
Star age | 4.27 |
Star temperature | 6020 |
Star alternate names | 2MASS J18590919+4435300, KIC 8480285, KOI-691, WISE J185909.19+443529.8 |
Wikipedia article | Kepler-647 b |
Back
| |
Fictional info (?) |
Suggested name | Ekyuge Kyo |
Planet type | Cold planet |
Ekyuge Kyo is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the valleys, deserts, and polar ice caps of Earth. Ekyuge Kyo is orbiting Kepler-647 every 16 Earth days. It has the longest rotation period (445 days) of any planet in its solar system and rotates in the opposite direction to most other planets.
When viewed from Homoshi, Ekyuge Kyo can reach an apparent magnitude of -3, bright enough for its reflected light to cast shadows, and making it on average the third-brightest object in the night sky. This cold planet is named after the deity Ekyuge Kyo, the bringer of destruction.
Its orbital eccentricity is the largest of all known planets in its solar system; at perihelion, Ekyuge Kyo's distance from Kepler-647 is only about two-thirds (or 69 pct) of its distance at aphelion.
Ekyuge Kyo is shrouded by an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light.
The Ekyuge Kyo system has a unique configuration among those of the planets because its axis of rotation is tilted sideways, nearly into the plane of its solar orbit. |
Atmosphere | Nitrogen | 66% |
Methane | 18% |
Sulfur dioxide | 10% |
Molecular hydrogen | 5.4% |
Atmospheric pressure | 0.4 bar |
|
Moon | Pyapano'kemo | Small irregular ice moon |
Konugogu | Medium-sized round rocky moon |
Jogyasa | Small round gaseous moon |
Nyunyu Moeryu | Small almost round rocky moon |
Kadamu Ryu | Medium-sized slightly egg-shaped rocky asteroid |
Toboapya-na | Large potato shaped rocky planetoid |
Uwabawo | Huge round rocky comet |
Pojazu Me | Large irregular ice planetoid |
Gakya | Medium-sized almost round ice moon |
Kyuju-ku | Small almost round gaseous comet |
Pyonu Kyogyo | Large round ice asteroid |
Yokebya | Small irregular rocky planetoid |
Hibyu Hyopi'shu | Large irregular gaseous moon |
Yanu Pera | Small irregular ice planetoid |
Jito | Very small round crater-filled asteroid |
Kaso-shu | Medium-sized almost round crater-filled comet |
Noeho Ke | Small round rocky comet |
Jitapyu Nyajo | Small irregular oceanic moon |
Hakishi Ge | Small almost round rocky asteroid |
Shihyu Chikyo Nya | Medium-sized slightly egg-shaped oceanic asteroid |
Shoshogya | Very small almost round gaseous asteroid |
Chui'serya | Medium-sized almost round gaseous moon |
Gumyo'tsu | Very small slightly egg-shaped gaseous comet |
Pyupagyu Romo | Huge almost round ice planetoid |
Google search for Ekyuge kyo |
|
Website by Joachim Michaelis
|
|
|
|