Kepler-38
Kepler-38 is a binary star system. These stars, called Kepler-38A and Kepler-38B have masses of 95% and 25% solar masses respectively. The brighter star is spectral class G while the secondary has spectral class M. They are separated by 0.147 AU, and complete an eccentric orbit around a common center of mass every 18.8 days.[4]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Lyra |
| Right ascension | 19h 07m 19.2814s[1] |
| Declination | +42° 16′ 45.120″[1] |
| Characteristics | |
| Spectral type | G / M[2] |
| Astrometry | |
| Proper motion (μ) | RA: −4.648±0.026[1] mas/yr Dec.: −13.159±0.025[1] mas/yr |
| Parallax (π) | 0.8225 ± 0.0145[1] mas |
| Distance | 3,970 ± 70 ly (1,220 ± 20 pc) |
| Orbit | |
| Primary | Kepler-38A |
| Companion | Kepler-38B |
| Period (P) | 18.79537 |
| Semi-major axis (a) | 0.1469 |
| Eccentricity (e) | 0.1032 |
| Details | |
| Kepler-38A | |
| Mass | 0.949 M☉ |
| Radius | 1.757 R☉ |
| Temperature | 5640 K |
| Metallicity | -0.11 |
| Kepler-38B | |
| Mass | 0.249 M☉ |
| Radius | 0.2724 R☉ |
| Metallicity | -0.11 |
| Other designations | |
| Database references | |
| SIMBAD | data |
| KIC | data |
Planetary system
In 2012, a circumbinary Neptune-sized planet was found transiting the brighter star. Follow-up radial velocity measurements did not give sufficient information to constrain the mass of the planet. The planet was confirmed via transit duration variation method.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | — | 0.4644 | 105.595 | — | — | 0.39 RJ |
gollark: ACTUAL feature suggestions?
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gollark: ```rust#[macro_use] extern crate serenity;use serenity::client::{Client, EventHandler};use serenity::framework::standard::StandardFramework;use std::env;struct Handler;impl EventHandler for Handler {}pub fn main() { // Login with a bot token from the environment let mut client = Client::new(&env::var("DISCORD_TOKEN").expect("token"), Handler) .expect("Error creating client"); client.with_framework(StandardFramework::new() .configure(|c| c.prefix("~")) .cmd("ping", ping)); if let Err(why) = client.start() { println!("An error occurred while running the client: {:?}", why); }}command!(ping(_context, message) { let _ = message.reply("Pong!");});```This is the example code, admittedly, yes.
gollark: It's in Rust.
gollark: AutoBotRobot is currently undergoing extensive development and testing. Feature suggestions?
References
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- "Notes for star Kepler-38(AB)". Extrasolar Planets Encyclopaedia. 2012. Retrieved 29 April 2013.
- "Kepler-38". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 January 2017.
- The Neptune-Sized Circumbinary Planet Kepler-38b, 18 August 2012 Jerome A. Orosz, William F. Welsh, Joshua A. Carter, Erik Brugamyer, Lars A. Buchhave, William D. Cochran, Michael Endl, Eric B. Ford, Phillip MacQueen, Donald R. Short, Guillermo Torres, Gur Windmiller, Eric Agol, Thomas Barclay, Douglas A. Caldwell, Bruce D. Clarke, Laurance R. Doyle, Daniel C. Fabrycky, John C. Geary, Nader Haghighipour, Matthew J. Holman, Khadeejah A. Ibrahim, Jon M. Jenkins, Karen Kinemuchi, Jie Li, Jack J. Lissauer, Andrej Prsa, Darin Ragozzine, Avi Shporer, Martin Still, Richard A. Wade
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