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Etymologie

Was (wer) ist BD 20 274 b - definition

STAR IN THE CONSTELLATION ARIES

BD plus 20 307; BD +20 307; BD +20deg307; HIC 8920; HIP 8920; SAO 75016; BD+20 307; BD+20° 307; BD +20° 307; BD +20°307

BD+20 274 b

BD+20 274 b is an exoplanet that was discovered in 2012. It has an orbital period of 578 days and has a mass 4 times larger than that of Jupiter.

https://en.wikipedia.org/wiki/BD+20_274_b

Heinkel He 274

PROTOTYPE BOMBER AIRCRAFT BY HEINKEL

He-274; He 274

The Heinkel He 274 was a German heavy bomber design developed during World War II, purpose-designed for high-altitude bombing with pressurized crew accommodation.

https://en.wikipedia.org/wiki/Heinkel_He_274

Bede BD-5

SPORT AIRCRAFT FAMILY BY JIM BEDE

BD-5J; Acro Star; Acrostar; Bede BD-5 Micro; Bede BD-5A; Bede BD-5B; Bede BD-5C; Bede BD-5D; Bede BD-5J; Bede BD-5S; FLS Microjet; Bede BD-5J Micro-Jet; Bede BD-5J Micro

The Bede BD-5 Micro is a series of small, single-seat homebuilt aircraft created in the late 1960s by US aircraft designer Jim Bede and introduced to the market primarily in kit form by the now-defunct Bede Aircraft Corporation in the early 1970s.

https://en.wikipedia.org/wiki/Bede_BD-5

Wikipedia

BD+20°307

BD+20°307 is a close binary star system approximately 300 light-years away in the constellation Aries. The system is surrounded by a dusty ring, and probably orbited by a 0.48M_☉ white dwarf on a wide (980 AU) orbit.

The dust that orbits around several hundred main-sequence stars is cold and comes from a Kuiper-belt analogous region. In the Solar System the ongoing collisions between asteroids generate a tenuous cloud of dust known as the zodiacal light. When the Solar System was young such collisions were more common and the rate of dust production was probably many times higher. Zodiacal dust around stars much younger than the Sun has been rarely found. Only a few main-sequence stars have revealed warm (>120 K) zodiacal dust.

An exceptionally large amount of warm, small, silicate dust particles around the solar-type star BD+20°307 (HIP 8920, SAO 75016) has been reported. The composition, quantity and temperature of the dust may be explained by recent, frequent or huge collisions between asteroids or other planetesimals whose orbits are being perturbed by a nearby planet.

https://en.wikipedia.org/wiki/BD+20°307