Estimates of galaxy numbers - re Herschel resuts

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Discussion Overview

The discussion revolves around estimates of the number of galaxies in the observable universe, particularly in relation to observations made by the Herschel Space Observatory. Participants explore the implications of these observations and compare them to other significant astronomical surveys, such as the Hubble Ultra Deep Field.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant mentions an article by Steve Eales that suggests imaging the entire celestial sphere with Herschel could imply around 23 million galaxies, prompting a question about the actual estimated total number of galaxies.
  • Another participant cites estimates of approximately 10^11 galaxies in the observable universe, noting that Herschel primarily observes relatively nearby galaxies, which may account for the lower number suggested by the first participant.
  • The Hubble Ultra Deep Field is referenced as a benchmark for galaxy counts, with about 10,000 galaxies observed in a very small portion of the sky, indicating a much larger total when extrapolated.
  • A participant expresses admiration for the Herschel image, highlighting its significance in showing galaxies whose light has traveled a significant portion of the universe's age.
  • There is a request for a link to the specific Herschel image, with suggestions for where to find it.
  • Another participant discusses the density of galaxies observed by Herschel, noting it represents only a fraction of the total density and reflects on why the night sky is not as bright as expected, attributing this to the processing of raw data and the effects of cosmic expansion.
  • The same participant speculates about the role of the Virial Theorem in understanding the dynamics of galaxy distributions and their gravitational interactions.

Areas of Agreement / Disagreement

Participants express varying estimates of the number of galaxies, with some agreeing on the rough figure of 10^11 while others propose different interpretations based on Herschel's observations. The discussion remains unresolved regarding the implications of these observations and the reasons behind the perceived brightness of the night sky.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about galaxy density and the effects of cosmic expansion on observed brightness. The calculations and interpretations of data from Herschel and Hubble are not fully resolved.

Paulibus
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In the January 2013 issue of Physics World there is an article by Steve Eales, illustrated with some remarkable images of galaxies obtained with the Herschel observatory. One, on page 31, is very appropriately captioned "Not stars; galaxies", because it looks very like star clouds, say in Sagittarius. It is a quite wonderful image that shows some 7000 galaxies; I'm told it's about four degrees on a side. If the entire celestial sphere were somehow to be imaged by Herschel in this way I figure one might say that the so observed universe would contain about 23 million galaxies. This prompts me to ask what, by comparison, is the actual estimated total number of galaxies in the observable galaxy-containing universe?
 
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Most estimates I have seen conclude that there are about 10^11 galaxies in the observable universe. This link (http://en.wikipedia.org/wiki/Observable_universe) goes through a couple of calculations. Of course this is a rough number.

Herschel is only seeing relatively nearby galaxies, which is why your number is so much smaller.
 
Thanks, Phyzguy and Chronos. For me, that Herschel image is as impressive in its way as the Hubble images, as it incudes galaxies whose light has taken about 3/4 of our universe's age to reach us. Regarding these as "relatively nearby galaxies" truly emphasizes the immensity of our astronomical environment!
 
link to the Herschel image please?

TIA,
Eric
 
Eric: I'm not sure if a link to this specific image is available. You could try herschel.cf.ac.uk or h-atlas.org which have lots of Herschel images.

physicsworld.com is the link to the magazine where the image was published in the January 2013 issue, p.31. I saw the print edition, but access to the link may need membership of the Inst. of Physics.
 
Ref the Cosmology thread, Estimating the number of galaxies, submitted by Jim Johnson
 
Thanks, jimjohnson,for pointing me to this
interesting thread . It fully answers my query about the total density of galaxies. The observed-by-Herschel density is only about 1/7000 part of this total but still gives the impression, rather like the star clouds in our Milky way, of an almost continuous, wall-to-wall distribution of galaxies. It first made me wonder why our night sky is not as bright as our Milky way --- galaxies are after all gravity-bound structures that don't expand along with the universe, so their per unit perceived- area surface brightness, like that of stars,
should be independent of distance from us. I now realize that my above impression must be an artefact of the way the raw Herschel data was processed, which masks the dimming produced by the galaxy separations created by the universe’s expansion. I suspect that this expansion may be ruled by the balance of energies mandated by the Virial Theorem, which rules many other dynamic activities, such as the height attained by stones we toss upwards, the speeds of orbiting planets in our solar system, and of both stars or galaxies that are gravitationally bound together. This theorem is a true vis viva of systems.
 

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