Examples of using Interstellar medium in English and their translations into Romanian
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The Interstellar Medium.
The ionized gas is expelled into the surrounding interstellar medium.
If you look out into the interstellar medium, the same compounds are there as on Earth.
Late in thelife of these stars, they ejected heavier elements into the interstellar medium.
The Local Bubble is a cavity in the interstellar medium(ISM) in the Orion Arm of the Milky Way.
The group plans to hide around the energy rich brown dwarfs in the interstellar medium.
Springing from the mysterious interstellar medium… the riddle of the nebulas is how they can form… from what is almost nothing at all.
It has also been found in the atmosphere of Venus,in the Hale-Bopp comet and in the interstellar medium.
Interstellar Medium The interstellar medium(or ISM) is the material that exists in the space between the stars.
Filling the distances between the Sun and all its galactic neighbors… is the neutral interstellar medium or lSM.
This cloud of material sweeps up the surrounding interstellar medium during a free expansion phase, which can last for up to two centuries.
And this is the Crab Nebula a stellar graveyard, where gas anddust are being dispersed back into the interstellar medium.
The particles in the interstellar medium… are ninety percent hydrogen atoms, ten percent helium… and trace amounts of other elements and tiny specks of dust.
Among the objects studied are the Sun, other stars, galaxies,extrasolar planets, the interstellar medium and the cosmic microwave background.
Heliopause===The heliosphere is divided into two regions; the solar wind travels at roughly 400 km/s until it collides with the interstellar wind;the flow of plasma in the interstellar medium.
The black lanes of gas anddust… show us where the interstellar medium… is clumping together to form nebulas in their most primeval form.
The outer limit of the solar wind's influence is roughly four times Pluto's distance from the Sun;this"heliopause" is considered the beginning of the interstellar medium.
Observations from the Herschel telescope revealed that the interstellar medium in our galaxy is threaded with filamentary structures of gas and dust on every scale.
Within a galaxy such as the Milky Way,atoms have a much higher concentration, with the density of matter in the interstellar medium(ISM) ranging from 105 to 109 atoms/m3.
The density of cosmic rays in the interstellar medium and the strength of the Sun's magnetic field change on very long timescales, so the level of cosmic-ray penetration in the Solar System varies, though by how much is unknown.
The gas expelled into space… as supernova remnants andplanetary nebulas… returns to the interstellar medium… where it becomes raw material for future generations of stars.
And doing this for 14 billion years, we end up with this picture,which is a very important graph, showing relative abundances of chemical elements in sun-like stars and in the interstellar medium.
A molecular form called protonated molecular hydrogen(H3+)is found in the interstellar medium(ISM), where it is generated by ionization of molecular hydrogen from cosmic rays.
This may be an upper limit to the age,because ejected material will be slowed when it encounters material ejected from the star at earlier stages of its evolution, and the interstellar medium.
Interstellar medium===A major issue with traveling at extremely high speeds is that interstellar dust and gas may cause considerable damage to the craft, due to the high relative speeds and large kinetic energies involved.
The collision occurs at the termination shock,which is roughly 80- 100 AU from the Sun upwind of the interstellar medium and roughly 200 AU from the Sun downwind.
Primordial nuclides were present in the interstellar medium from which the solar system was formed, and were formed in, or after, the Big Bang, by nucleosynthesis in stars and supernovae followed by mass ejection, by cosmic ray spallation, and potentially from other processes.
The wave then gradually undergoes a period of adiabatic expansion, andwill slowly cool and mix with the surrounding interstellar medium over a period of about 10,000 years.
Planetary nebulae play a crucial role in the chemical evolution of the galaxy,returning material to the interstellar medium that has been enriched in heavy elements and other products of nucleosynthesis( such as carbon, nitrogen, oxygen and calcium).
Ln fact, our own bodies are made out of recycled material… from earlier generations of stars… that had dispersed material into the interstellar medium… before our own solar system formed.