FACTOID # 10: The total number of state executions in 2005 was 60: 19 in Texas and 41 elsewhere. The racial split was 19 Black and 41 White.
 
 Home   Encyclopedia   Statistics   States A-Z   Flags   Maps   FAQ   About 
   
 
WHAT'S NEW
 

SEARCH ALL

FACTS & STATISTICS    Advanced view

Search encyclopedia, statistics and forums:

 

 

(* = Graphable)

 

 


Encyclopedia > Hubble constant

Hubble's law is the statement in astronomy that the redshift in light coming from distant galaxies is proportional to their distance. The law was first formulated by Edwin Hubble in 1929.


If one assumes that this redshift is caused by Doppler effect while galaxies move away from us then it leads to a picture of an expanding universe and, by extrapolating back in time, to the Big Bang theory. Hubble compared the distances to nearby galaxies to their redshift, found a linear relationship. His estimate of the proportionality constant, known as Hubble's constant (and now also as "Hubble's parameter" since it turned out to be not a constant but a parameter that depends on time in a way suggesting accelerating expansion of the universe), was however off by a factor of about 10. Furthermore, if one takes Hubble's original observations and then uses the most accurate distances and velocities currently known, one ends up with a random scatter plot with no discernable relationship between redshift and distance. Nevertheless an approximately linear relationship between redshift and distance was confirmed by observations after Hubble. The law can be stated as follows:

v = H0 D

where v is the redshift, typically expressed in km/s (velocity that the galaxy should move with, away from us, to produce this redshift through Doppler effect), H0 is Hubble's parameter (at the observer, as denoted by the subscript), and D is the current distance from the observer to the galaxy, measured in megaparsecs: Mpc.


One can derive Hubble's law mathematically if one assumes that the universe expands (or shrinks) and that the universe is homogeneous, meaning that all points within it are equal.


For most of the second half of the 20th century the value of H0 was estimated to be between 50 and 90 km/s/Mpc. The value of the Hubble constant was the topic of a long and rather bitter controversy between Gérard de Vaucouleurs who claimed the value was 100 and Allan Sandage who claimed the value was 50. The Hubble Key Project significantly improved the determination of the value and in May 2001 published its final estimate of 72+/-8  km/s/Mpc. In 2003 the satellite WMAP further improved that determination to 71+/-4, using a completely independent method, based in the measurement of anisotropies in the cosmic microwave background radiation.


Hubble's constant is "constant" in the sense that it is believed to work for all velocities and distances right now. The value of H (usually called Hubble parameter to distiguish it from its value now, the Hubble constant) decreases over time however. If one assumes that all galaxies retain their speed relative to us and do not accelerate or decelerate, then we have D = vt and it follows that H = 1/t, where t is the time since the Big Bang. This allows to estimate the age of the universe from H.


Based on recent observations, it is now believed that galaxies accelerate away from us, which means that H > 1/t (but still decreases over time) and the estimate 1/H0 (between 11 and 20 billion years) for the age of the universe is too low.


There are several additional notes to be made:

  • The distance D to nearby galaxies can be estimated for example by comparing their apparent luminosity to their postulated absolute luminosity.

If the galaxies are far away, one has to take as D the distance to the galaxy right now, not when the light from it was emitted. This distance is extremely hard to determine.

  • The velocity v is defined to be the time rate of change of D.

For relatively nearby galaxies, the velocity v can be determined from the galaxy's redshift z using the formula vzc where c is the speed of light. However, only the velocity due to the expansion of the universe should be used: all galaxies move relative to each other independent of the expansion of the universe, and these relative velocities, called peculiar velocities are not accounted for by Hubble's law. For far away galaxies, v cannot easily be determined from the redshift z and can be larger than c.

  • Systems that are gravitationally bound, such as galaxies or our planetary system, are not subject to Hubble's law and do not expand.

See also

External links and references


  Results from FactBites:
 
Hubble's law - Wikipedia, the free encyclopedia (1386 words)
Hubble's law is the statement in physical cosmology that the redshift in light coming from distant galaxies is proportional to their distance.
Though there was considerable scatter (now known to be due to peculiar velocities), Hubble was able to plot a trend line from the 46 galaxies he studied and obtained a value for the Hubble constant of approximately 400 km/s/Mpc, which is much higher than the currently accepted value due to errors in his distance calibrations.
The value of the Hubble constant was the topic of a long and rather bitter controversy between GĂ©rard de Vaucouleurs who claimed the value was 100 and Allan Sandage who claimed the value was 50.
Hubble Constant (1451 words)
The value of the Hubble Constant is important for both observations of the objects in the Universe, as it allows us to convert their recession velocities into true distances, and for estimating the age of the Universe.
Below is shown Hubble's original figure from the 1929 paper - where he plotted the radial velocities in km/sec of the galaxies against his estimates of their distances (in parsecs) derived from the apparent magnitudes of what he thought were the bright supergiant stars.
Hubble Space Telescope were to use it to measure the sizes of distant galaxies and to detect the variations in the luminosity of variable stars in distant galaxies.
  More results at FactBites »

 
 

COMMENTARY     


Share your thoughts, questions and commentary here
Your name
Your comments

Want to know more?
Search encyclopedia, statistics and forums:

 


Press Releases |  Feeds | Contact
The Wikipedia article included on this page is licensed under the GFDL.
Images may be subject to relevant owners' copyright.
All other elements are (c) copyright NationMaster.com 2003-5. All Rights Reserved.
Usage implies agreement with terms, 1022, m