Refined Hubble Constant narrows explanations for dark energy

May 7, 2009
This is a Hubble Space Telescope photo of the spiral galaxy NGC 3021. This was one of several hosts of recent Type Ia supernovae observed by astronomers to refine the measure of the universe's expansion rate, called the Hubble constant. Hubble made precise measurements of Cepheid variable stars in the galaxy, highlighted by green circles in the four inset boxes. These stars pulsate at a rate that is matched closely to their intrinsic brightness. This makes them ideal for measuring intergalactic distances. The Cepheids are used to calibrate an even brighter milepost marker that can be used over greater distances, a Type Ia supernova. The supernova was observed in the galaxy in 1995. The images in the boxes were taken with the Near Infrared Camera and Multi-Object Spectrometer (NICMOS).

Whatever dark energy is, explanations for it have less wiggle room following a Hubble Space Telescope observation that has refined the measurement of the universe's present expansion rate to a precision where the error is smaller than 5 percent. The new value for the expansion rate, known as the Hubble constant, or Ho (after Edwin Hubble who first measured the expansion of the universe nearly a century ago), is 74.2 kilometers per second per megaparsec (error margin of ± 3.6). The results agree closely with an earlier measurement gleaned from Hubble of 72 ± 8 km/sec/megaparsec, but are now more than twice as precise.

The Hubble measurement, conducted by the SHOES (Supernova Ho for the Equation of State) Team and led by Adam Riess, a professor in the Henry A. Rowland Department of Physics and Astronomy at Johns Hopkins University's Krieger School of Arts and Sciences and at the Space Telescope Science Institute, uses a number of refinements to streamline and strengthen the construction of a cosmic "distance ladder," a billion light-years in length, that astronomers use to determine the universe's expansion rate.

Hubble observations of pulsating stars called Cepheid variables in a nearby cosmic mile marker, the galaxy NGC 4258, and in the host galaxies of recent supernovae, directly link these distance indicators. The use of Hubble to bridge these rungs in the ladder eliminated the systematic errors that are almost unavoidably introduced by comparing measurements from different telescopes.

Riess explains the new technique: "It's like measuring a building with a long tape measure instead of moving a yard stick end over end. You avoid compounding the little errors you make every time you move the yardstick. The higher the building, the greater the error."

Lucas Macri, professor of physics and astronomy at Texas A&M, and a significant contributor to the results, said, "Cepheids are the backbone of the distance ladder because their pulsation periods, which are easily observed, correlate directly with their luminosities. Another refinement of our ladder is the fact that we have observed the Cepheids in the near-infrared parts of the electromagnetic spectrum where these variable stars are better distance indicators than at optical wavelengths."

This new, more precise value of the Hubble constant was used to test and constrain the properties of dark energy, the form of energy that produces a repulsive force in space, which is causing the expansion rate of the universe to accelerate.

By bracketing the expansion history of the universe between today and when the universe was only approximately 380,000 years old, the astronomers were able to place limits on the nature of the dark energy that is causing the expansion to speed up. (The measurement for the far early universe is derived from fluctuations in the cosmic microwave background, as resolved by NASA's Wilkinson Microwave Anisotropy Probe, WMAP, in 2003.)

Their result is consistent with the simplest interpretation of dark energy: that it is mathematically equivalent to Albert Einstein's hypothesized cosmological constant, introduced a century ago to push on the fabric of space and prevent the universe from collapsing under the pull of gravity. (Einstein, however, removed the constant once the expansion of the universe was discovered by Edwin Hubble.)

"If you put in a box all the ways that dark energy might differ from the cosmological constant, that box would now be three times smaller," says Riess. "That's progress, but we still have a long way to go to pin down the nature of dark energy."

Though the cosmological constant was conceived of long ago, observational evidence for dark energy didn't come along until 11 years ago, when two studies, one led by Riess and Brian Schmidt of Mount Stromlo Observatory, and the other by Saul Perlmutter of Lawrence Berkeley National Laboratory, discovered dark energy independently, in part with Hubble observations. Since then astronomers have been pursuing observations to better characterize dark energy.

Riess's approach to narrowing alternative explanations for dark energy--whether it is a static cosmological constant or a dynamical field (like the repulsive force that drove inflation after the big bang)--is to further refine measurements of the universe's expansion history.

Before Hubble was launched in 1990, estimates of the Hubble constant varied by a factor of two. In the late 1990s the Key Project on the Extragalactic Distance Scale refined the value of the Hubble constant to an error of only about 10 percent. This was accomplished by observing Cepheid variables at optical wavelengths out to greater distances than obtained previously and comparing those to similar measurements from ground-based telescopes.

The SHOES team used Hubble's Near Infrared Camera and Multi-Object Spectrometer (NICMOS) and the Advanced Camera for Surveys (ACS) to observe 240 Cepheid variable stars across seven galaxies. One of these galaxies was NGC 4258, whose distance was very accurately determined through observations with radio telescopes. The other six galaxies recently hosted Type Ia supernovae that are reliable distance indicators for even farther measurements in the universe. Type Ia supernovae all explode with nearly the same amount of energy and therefore have almost the same intrinsic brightness.

By observing Cepheids with very similar properties at near-infrared wavelengths in all seven , and using the same telescope and instrument, the team was able to more precisely calibrate the luminosity of supernovae. With Hubble's powerful capabilities, the team was able to sidestep some of the shakiest rungs along the previous distance ladder involving uncertainties in the behavior of Cepheids.

Riess would eventually like to see the Hubble constant refined to a value with an error of no more than 1 percent, to put even tighter constraints on solutions to .

Source: Johns Hopkins University (news : web)

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3.3 / 5 (4) May 07, 2009
It's quintessence! Seriously now! Why is it so hard to take the "novel" out of this idea and make it available to scholars as a rather sensible option? We know that the Big Bang wasn't an explosion; it was expansion after inflation - as it still is - but why can we not draw the same lines for an ethereal medium that we can for a gaseous one when material/energy is ejected outward? What makes more sense: (1) everything expanding into *nothing*, or (2) everything expanding into a matrix of which we do not have the instruments to properly measure yet? We can see it's effects... and it would be logical to theorize that homogeneity and anisotropic isotropies, as well as uniform matter dispersal, are all due to luminescent and dark matter traveling through a medium which does not interact! The scale factor would be a sign that all matter is spreading into a 'dark energy' universe and is becoming a weak suspension. Bang!
2 / 5 (4) May 07, 2009
And a boojum is a particularly viscous type of snark.
1 / 5 (2) May 07, 2009
A particularly *dangerous* kind of snark, sure. I would surmise that you're either being humorous, or suggestive that superfluids have something to do with the Hubble Constant and dark energy?
1 / 5 (2) May 07, 2009
As chicken feet are to Wylie E. Coyote....
3 / 5 (3) May 07, 2009
1 / 5 (3) May 07, 2009
I wonder if the superfluid gravastar theory is knocked out by the discoveries of our universe's dodecahedral framework. I, for one, do not believe that dark energy interacts with any matter (unlike the assumptions of said theory); it seems, moreso, to be the non-intrusive medium which this - and perhaps other - simultaneous/past expansions can move in. To claim it is a violation of quantum theory that light's energy increases when it enters an event horizon is equally strange. We can slow it down in labs. If the gravitational magnitude of any black hole is strong enough to "drag it" faster than it hauls naturally, I don't think that's a 'violation.' But hey. I'm just a college student!
1 / 5 (2) May 07, 2009
1 / 5 (2) May 08, 2009
If a body presents itself to our telescopes from a distance close to the BB, how come we got here first, to be in position to see its incoming photons?
3 / 5 (1) May 08, 2009
well... there was no center of expansion, as there is with an explosion. The CMB shows us this. It happened, and is still happening, everywhere at once. It's just the matter that objects "out there" are visibly expanding "faster" because of the scale factor... and it takes a while for the light from it all to get to us, because inflation really sent things out there.
1 / 5 (1) May 08, 2009
The formation of matter is endlessly going on using vacuum energy.The newly born matter is pushing the existing matter away in the whole universe.So the universe is inflating endlessly,but the space will not be more empty because the newly borne matter fills it.
5 / 5 (1) May 10, 2009
Kairos: From your first post, I don't know if this will answer your question, but if I am reading it correctly, the possibility has been looked into.


This article describes an idea that our universe exists in the middle of an area of lower density. Our universe is getting pulled towards the regions of higher density, which looks like the dark energy acceleration we observe.
not rated yet Jun 14, 2009
what if those high temp darkmatter filaments that connect starclusters, galaxies, ...superclusters, are so hot because the DM is going at near C velocities along these tunnels. If the antigrav beam theory is right, ( http://www.physor...789.html ) that could be doing the pushin'.
Maybe they are coaxial spacetime tunnels for high speed travel between stars and galaxies?
Could be where those more than 10^19 GeV cosmic rays come from.

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