outer space - translation to greek
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  3. outer space

outer space - translation to greek

VOID BETWEEN CELESTIAL BODIES
Interstellar space; Outer Space; Intergalactic gas; Intergalactic space; Edge of space; Boundary to space; Cislunar space; Deepspace; Cislunar; Space boundary; Space border; Geospace; Inter-planetary space; Cis-lunar space; Cislunar medium; Space/universe; Outer-space; Spaceborne; Space-borne; Space-based; XGEO; Near-Earth space
  • alt=Patchy orange and blue nebulosity against a black background, with a curved orange arc wrapping around a star at the center.
  • Earth and the Moon as seen from cislunar space
  • first image taken by a human of the whole Earth]], probably photographed by [[William Anders]] of [[Apollo 8]].<ref name="Apollo8FlightJournalDay1"/> South is up; South America is in the middle.
  • alt=The lower half shows a blue planet with patchy white clouds. The upper half has a man in a white spacesuit and maneuvering unit against a black background.
  • inflation]] from the initial state, followed thereafter by steadier expansion to the present day, shown at right.
  • alt=At lower left, a white coma stands out against a black background. Nebulous material streams away to the top and left, slowly fading with distance.
  • geosynchronous]] and [[low Earth orbit]]
  • the atmosphere]] are drawn to scale, whereas objects within them, such as the [[International Space Station]], are not.
  • The [[interplanetary dust cloud]] illuminated and visible as [[zodiacal light]], with its parts the ''false dawn'',<ref name=eso_2017/> ''[[gegenschein]]'' and the rest of its band, which is visually crossed by the [[Milky Way]]
  • alt=A black background with luminous shapes of various sizes scattered randomly about. They typically have white, red or blue hues.
  • abbr=on}} altitude in [[low Earth orbit]]. In the background the [[Milky Way]]'s [[interstellar space]] is visible, as well as in the foreground, above Earth, the [[airglow]] of the [[ionosphere]] just below and beyond the so-defined edge of space the [[Kármán line]] in the [[thermosphere]].
  • Aurora australis]] observed from the [[International Space Station]]
  • alt=A glass display case holds a mechanical device with a lever arm, plus two metal hemispheres attached to draw ropes
  • alt=At top, a dark rocket is emitting a bright plume of flame against a blue sky. Underneath, a column of smoke is partly concealing a navy ship.
  • alt=A white rocketship with oddly-shaped wings at rest on a runway.
  • cosmic voids]] of the intergalactic medium.

outer space         
απώτερο διάστημα
space time         
  • '''here''']].
  • Figure 2–9. In this spacetime diagram, the 1&nbsp;m length of the moving rod, as measured in the primed frame, is the foreshortened distance OC when projected onto the unprimed frame.
  • Figure 4-4. Dewan–Beran–Bell spaceship paradox
  • Figure 4–5. The curved lines represent the world lines of two observers A and B who accelerate in the same direction with the same constant magnitude acceleration. At A' and B', the observers stop accelerating. The dashed lines are lines of simultaneity for either observer before acceleration begins and after acceleration stops.
  • Figure 3–9. Energy and momentum of light in different inertial frames
  • Figure 5–9. (A) Cavendish experiment, (B) Kreuzer experiment
  • Figure 3–5. Derivation of Lorentz Transformation
  • Figure 5–3. Einstein's argument suggesting gravitational redshift
  • Figure 5–2. Equivalence principle
  • Figure 3–1. '''Galilean''' Spacetime and composition of velocities
  • Figure 2–3. (a) Galilean diagram of two frames of reference in standard configuration, (b) spacetime diagram of two frames of reference, (c) spacetime diagram showing the path of a reflected light pulse
  • '''Click here to animate.''']]
  • Figure 5-11. Gravity Probe B confirmed the existence of gravitomagnetism
  • Figure 2-11. Spacetime explanation of the twin paradox
  • Figure 3–4. Lorentz factor as a function of velocity
  • Figure 1–4. Hand-colored transparency presented by Minkowski in his 1908 ''Raum und Zeit'' lecture
  • Figure 2–4. The light cone centered on an event divides the rest of spacetime into the future, the past, and "elsewhere"
  • Figure 1-1. Each location in spacetime is marked by four numbers defined by a [[frame of reference]]: the position in space, and the time (which can be visualized as the reading of a clock located at each position in space). The 'observer' synchronizes the clocks according to their own reference frame.
  • 1=''2'' and ''3''}} really represent tidal effects resulting from their differential attraction by mass&nbsp;''1''. (iii) A third reporter, trained in general relativity, knows that there are, in fact, no forces at all acting between the three objects. Rather, all three objects move along [[geodesics]] in spacetime.</ref>
  • Figure 3–2. Relativistic composition of velocities
  • Figure 3-10. Relativistic conservation of momentum
  • Figure 3–8. Relativistic spacetime momentum vector
  • Figure 2–6. Animation illustrating relativity of simultaneity
  • tanh]]). Sinh is red, cosh is blue and tanh is green.
  • Figure 2–7. (a) Families of invariant hyperbolae, (b) Hyperboloids of two sheets and one sheet
  • Figure 3–6. Spacetime diagram of relativistic Doppler effect
  • Figure 2–1. Spacetime diagram illustrating two photons, A and B, originating at the same event, and a slower-than-light-speed object, C
  • Figure 3-3. Spacetime diagrams illustrating time dilation and length contraction
  • Figure 2–8. The invariant hyperbola comprises the points that can be reached from the origin in a fixed proper time by clocks traveling at different speeds
  • Figure 5–7. Origin of gravitomagnetism
  • Figure 2-2. Galilean diagram of two frames of reference in standard configuration
  • Figure 5-5. Contravariant components of the stress–energy tensor
  • Figure 3–7. Transverse Doppler effect scenarios
  • Figure 2–5. Light cone in 2D space plus a time dimension
MATHEMATICAL MODEL COMBINING SPACE AND TIME
Space-time interval; Spacetime interval; Time-space continuum; Space-like; Timelike; Spacelike; Light-like; Space-time continuum; Time-like; Space and time; Spacetime continuum; Neo newtonian; Neo-newtonian; Space/time continuum; Spacetime Interval; Space/time; Space time continueum; Interval spacetime; Space-time distance; Space time continuum; Invariant interval; Space time; Time space continuum; Time- space curvature; Space-Time; Space Time Continuum; Spacetimes; Lorentz interval; Time and space; Time and Space; Space–time; Space-time; Space-Time Continuum; Space–time continuum; Spacetime geometry; Draft:Spacetime; Spatiotemporal; Space Time; Spacetime (mathematics)
χωρόχρονος
space travel         
WIKIMEDIA DISAMBIGUATION PAGE
Space Travel; Space travel (disambiguation)
διαστημικό ταξίδι

Definition

outer space
¦ noun the physical universe beyond the earth's atmosphere.
Show more definitions

Wikipedia

Outer space

Outer space, commonly shortened to space, is the expanse that exists beyond Earth and its atmosphere and between celestial bodies. Outer space is not completely empty; it is a near-perfect vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium, as well as electromagnetic radiation, magnetic fields, neutrinos, dust, and cosmic rays. The baseline temperature of outer space, as set by the background radiation from the Big Bang, is 2.7 kelvins (−270 °C; −455 °F).

The plasma between galaxies is thought to account for about half of the baryonic (ordinary) matter in the universe, having a number density of less than one hydrogen atom per cubic metre and a kinetic temperature of millions of kelvins. Local concentrations of matter have condensed into stars and galaxies. Intergalactic space takes up most of the volume of the universe, but even galaxies and star systems consist almost entirely of empty space. Most of the remaining mass-energy in the observable universe is made up of an unknown form, dubbed dark matter and dark energy.

Outer space does not begin at a definite altitude above Earth's surface. The Kármán line, an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. Certain portions of the upper stratosphere and the mesosphere are sometimes referred to as "near space". The framework for international space law was established by the Outer Space Treaty, which entered into force on 10 October 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.

Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights. This was followed by crewed rocket flights and, then, crewed Earth orbit, first achieved by Yuri Gagarin of the Soviet Union in 1961. The economic cost of putting objects, including humans, into space is very high, limiting human spaceflight to low Earth orbit and the Moon. On the other hand, uncrewed spacecraft have reached all of the known planets in the Solar System. Outer space represents a challenging environment for human exploration because of the hazards of vacuum and radiation. Microgravity has a negative effect on human physiology that causes both muscle atrophy and bone loss.

https://en.wikipedia.org/wiki/Outer space
Examples of use of outer space
1. Otherwise, collisions would occur in outer space.
2. The treaty bans the stationing of weapons of mass destruction in outer space and declares outer space should be used only for peaceful purposes.
3. We are against the weaponisation of outer space," he said.
4. No specified country should be allowed to monopolize outer space.
5. McCartney‘s fame apparently even stretches to outer space.
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