gullible$33142$ - translation to ολλανδικά
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gullible$33142$ - translation to ολλανδικά

WIKIMEDIA LIST ARTICLE
List of stars with known planetary systems; List of stars with confirmed planets; List of stars with multiple exoplanets; List of stars with planets; List of stars with exoplanets; List of stars with extrasolar planets; List of stars with confirmed extrasolar planets; List of exoplanetary host stars; List of planetary systems; List of solar systems; Multiplanetary system; Muiltiplanets system; Multiplanet system; Multiplanets system; Exo Solar System; ExoSolar System; Exo-Solar System; Exosolar system; Extra-solar system; ExoSolarSystem; Extrasolarsystem; Kepler-55; HD 31527; HD 38677; TOI-763; K2-302; TOI-125; Kepler-446; EPIC 251319382; K2-37; K2-38; Kepler-100; K2-268; K2-183; Kepler-1542; K2-299; Kepler-92; Kepler-1388; K2-282; Kepler-1047; Kepler-1254; Kepler-289; Kepler-603; Kepler-758; Kepler-48; Kepler-49; Kepler-52; Kepler-53; Kepler-54; Kepler-58; Kepler-60; Kepler-79; Kepler-81; Kepler-82; Kepler-83; Kepler-85; Kepler-87; Kepler-106; Kepler-114; Kepler-122; Kepler-169; Kepler-238; Kepler-276; Kepler-279; Kepler-282; Kepler-292; Kepler-305; Kepler-350; Kepler-154; Kepler-304; Kepler-351; Kepler-166; Kepler-157; Kepler-342; Kepler-148; Kepler-403; Kepler-401; Kepler-398; Kepler-255; Kepler-245; Kepler-271; Kepler-132; Kepler-171; Kepler-127; Kepler-164; Kepler-130; Kepler-126; Kepler-104; Kepler-247; Kepler-197; Kepler-338; Kepler-454; Kepler-450; Kepler-176; Kepler-191; Kepler-192; Kepler-217; Kepler-218; Kepler-431; Kepler-399; Kepler-159; Kepler-150; Kepler-149; Kepler-142; Kepler-124; Kepler-402; Kepler-374; Kepler-372; Kepler-363; Kepler-359; Kepler-357; Kepler-354; Kepler-206; Kepler-203; Kepler-194; Kepler-184; Kepler-178; Kepler-336; Kepler-334; Kepler-332; Kepler-331; Kepler-327; Kepler-326; Kepler-325; EPIC 201085153; Kepler-172; OGLE-2012-BLG-0026L; Kepler-220; Kepler-221; Kepler-224; Kepler-208; Kepler-215; Kepler-235; Kepler-251; Kepler-256; Kepler-265; Kepler-286; Kepler-299; Kepler-306; Kepler-341; Kepler-339; Kepler-770; EPIC 249893012; Kepler-198; Kepler-267; Kepler-257; Kepler-254; Kepler-253; Kepler-250; Kepler-249; Kepler-207; Kepler-219; Kepler-222; Kepler-226; Kepler-272; Kepler-275; Kepler-228; Kepler-229; Kepler-244; Kepler-288; Kepler-295; Kepler-298; Kepler-301; Kepler-310; Kepler-319; K2-368; K2-381; K2-384; TOI-1246; HIP 34269; HD 28109; HD 33142; Gliese 3138; LP 358-499; HD 23472; K2-219; TOI-1136
  • microlensing]]}}

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gullible      
adj. makkelijk beet te nemen; onnozel

Ορισμός

gullible
a.
(Colloq.) Credulous, easily duped.

Βικιπαίδεια

List of multiplanetary systems

From the total of 3,943 stars known to have exoplanets (as of April 1, 2023), there are a total of 855 known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are Sol (the Solar System's star, also referred to as the Sun) and Kepler-90 with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets.

The 855 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d). The nearest system with four or more confirmed planets is Tau Ceti, with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 ly away.

The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important stellar properties are mass and metallicity because they determine how these planetary systems form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 AU.