hypervelocity - translation to russian
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hypervelocity - translation to russian

VERY HIGH VELOCITY
Hypervelocity impact
  • The aftermath of a hypervelocity impact, with a projectile the same size as the one that impacted for scale
  • The "energy flash" of a hypervelocity impact during a laboratory simulation of what happens when a piece of [[orbital debris]] hits a spacecraft in orbit

hypervelocity         

[haipəvi'lɔsiti]

существительное

общая лексика

гиперзвуковая скорость

космическая скорость

stellar motion         
  • Expected motion of 40,000 stars in the next 400 thousand years, as determined by Gaia EDR3
  • Four runaway stars plowing through regions of dense interstellar gas and creating bright bow waves and trailing tails of glowing gas. The stars in these NASA Hubble Space Telescope images are among 14 young runaway stars spotted by the Advanced Camera for Surveys between October 2005 and July 2006.
  • Monoceros]]
  • Relation between proper motion and velocity components of an object. At emission, the object was at distance ''d'' from the Sun, and moved at angular rate ''μ'' radian/s, that is, ''μ = v<sub>t</sub> / d'' with ''v<sub>t</sub>'' = the component of velocity transverse to line of sight from the Sun. (The diagram illustrates an angle ''μ'' swept out in unit time at tangential velocity ''v<sub>t</sub>''.)
  • Runaway star speeding from 30 Doradus. Image taken by the Hubble Space Telescope.
  • Gaia]]'', overlaid on top of an artistic view of the Milky Way
  • [[Ursa Major Moving Group]], the closest stellar moving group to Earth
STUDY OF THE MOVEMENT OF STARS
Moving cluster; Moving group; Runaway star; Hypervelocity star; Exiled stars; Exile stars; Runaway stars; Hypervelocity stars; OB association; Moving groups; High-velocity star; Stellar Associations; Stellar motion; Star association; Hyper-velocity star; Stellar stream; Space velocity (astronomy); Star streaming; Stellar kinematic group; Hercules-Lyra association; Hyper Velocity Stars; Stellar motions; High-velocity stars; HV*; High velocity stars; High velocity star

общая лексика

движение звезд

runaway star         
  • Expected motion of 40,000 stars in the next 400 thousand years, as determined by Gaia EDR3
  • Four runaway stars plowing through regions of dense interstellar gas and creating bright bow waves and trailing tails of glowing gas. The stars in these NASA Hubble Space Telescope images are among 14 young runaway stars spotted by the Advanced Camera for Surveys between October 2005 and July 2006.
  • Monoceros]]
  • Relation between proper motion and velocity components of an object. At emission, the object was at distance ''d'' from the Sun, and moved at angular rate ''μ'' radian/s, that is, ''μ = v<sub>t</sub> / d'' with ''v<sub>t</sub>'' = the component of velocity transverse to line of sight from the Sun. (The diagram illustrates an angle ''μ'' swept out in unit time at tangential velocity ''v<sub>t</sub>''.)
  • Runaway star speeding from 30 Doradus. Image taken by the Hubble Space Telescope.
  • Gaia]]'', overlaid on top of an artistic view of the Milky Way
  • [[Ursa Major Moving Group]], the closest stellar moving group to Earth
STUDY OF THE MOVEMENT OF STARS
Moving cluster; Moving group; Runaway star; Hypervelocity star; Exiled stars; Exile stars; Runaway stars; Hypervelocity stars; OB association; Moving groups; High-velocity star; Stellar Associations; Stellar motion; Star association; Hyper-velocity star; Stellar stream; Space velocity (astronomy); Star streaming; Stellar kinematic group; Hercules-Lyra association; Hyper Velocity Stars; Stellar motions; High-velocity stars; HV*; High velocity stars; High velocity star
убегающая звезда

Wikipedia

Hypervelocity

Hypervelocity is very high velocity, approximately over 3,000 meters per second (6,700 mph, 11,000 km/h, 10,000 ft/s, or Mach 8.8). In particular, hypervelocity is velocity so high that the strength of materials upon impact is very small compared to inertial stresses. Thus, metals and fluids behave alike under hypervelocity impact. Extreme hypervelocity results in vaporization of the impactor and target. For structural metals, hypervelocity is generally considered to be over 2,500 m/s (5,600 mph, 9,000 km/h, 8,200 ft/s, or Mach 7.3). Meteorite craters are also examples of hypervelocity impacts.

Examples of use of hypervelocity
1. The discovery of the two newest hypervelocity stars was no accident.
2. The team used data from the Sloan Digital Sky Survey as the starting point for its hypervelocity star search.
3. Then, in November and December, two separate groups of European astronomers published their detections of another hypervelocity star each.
4. Taking stars‘ measurements The two latest hypervelocity stars, however, clearly came from the Milky Way, Brown says.
5. DRAMATIC EXIT: Astronomers have identified a new class of objects called ‘hypervelocity stars.‘ This drawing shows one flung from the Milky Way‘s center, exiting the galaxy.
What is the Russian for hypervelocity? Translation of &#39hypervelocity&#39 to Russian