TR tube - significado y definición. Qué es TR tube
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Qué (quién) es TR tube - definición

BINARY STAR IN THE CONSTELLATION CARINA
OGLE-TR-122b; OGLE-TR 122; OGLE-TR 122b; OGLE-TR 122B; OGLE-TR-122B; OGLE TR 122; OGLE TR 122b; OGLE TR 122B; OGLE TR-122; OGLE TR-122b; OGLE TR-122B; OGLE-tr-122b; V817 Carinae
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Tube (container)         
SOFT, SQUEEZABLE CONTAINER WHICH CAN BE USED FOR THICK LIQUIDS SUCH AS ADHESIVE, CAULKING, OINTMENT, AND TOOTHPASTE
Toothpaste tube; Tube (packaging); Collapsible tube; Squeeze tube
A tube, squeeze tube, or collapsible tube is a collapsible package which can be used for viscous liquids such as toothpaste, artist's paint, adhesive, caulk, & ointments. Basically, a tube is a cylindrical, hollow piece with a round or oval profile, made of plastic, paperboard, aluminum, or other metal.
Tubeworm         
INDEX OF ANIMALS WITH THE SAME COMMON NAME
Tube worm (body plan); Tubeworm; Tube Worm; Tubeworms; Tube worms
·noun Any annelid which constructs a tube; one of the Tubicolae.
Tube worm         
INDEX OF ANIMALS WITH THE SAME COMMON NAME
Tube worm (body plan); Tubeworm; Tube Worm; Tubeworms; Tube worms
A tubeworm is any worm-like sessile invertebrate that anchors its tail to an underwater surface and secretes around its body a mineral tube, into which it can withdraw its entire body.

Wikipedia

OGLE-TR-122

OGLE-TR-122 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 7.3 days. The system's primary is thought to resemble the Sun.

The smaller star, OGLE-TR-122B, is estimated to have a radius around 0.12 solar radii, or around 20% larger than Jupiter's, and a mass of around 0.1 solar masses, or approximately 100 times Jupiter's. This makes its average density approximately 50 times the Sun's or over 80 times the density of water. OGLE-TR-122b's mass is close to the lowest possible mass for a hydrogen-fusing star, estimated to be around 0.07 or 0.08 solar masses. The observed transit provides the first direct evidence for a star with a radius comparable to Jupiter's.