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New Hubble constant measurement adds to mystery of universe's expansion rate
phys.org ^ | July 16, 2019 | by NASA's Goddard Space Flight Center

Posted on 07/16/2019 10:11:43 AM PDT by Red Badger

These galaxies are selected from a Hubble Space Telescope program to measure the expansion rate of the universe, called the Hubble constant. The value is calculated by comparing the galaxies' distances to the apparent rate of recession away from Earth (due to the relativistic effects of expanding space). By comparing the apparent brightnesses of the galaxies' red giant stars with nearby red giants, whose distances were measured with other methods, astronomers are able to determine how far away each of the host galaxies are. This is possible because red giants are reliable milepost markers because they all reach the same peak brightness in their late evolution. And, this can be used as a "standard candle" to calculate distance. Hubble's exquisite sharpness and sensitivity allowed for red giants to be found in the stellar halos of the host galaxies. The red giants were searched for in the halos of the galaxies. The center row shows Hubble's full field of view. The bottom row zooms even tighter into the Hubble fields. The red giants are identified by yellow circles. Credit: NASA, ESA, W. Freedman (University of Chicago), ESO, and the Digitized Sky Survey

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Astronomers have made a new measurement of how fast the universe is expanding, using an entirely different kind of star than previous endeavors. The revised measurement, which comes from NASA's Hubble Space Telescope, falls in the center of a hotly debated question in astrophysics that may lead to a new interpretation of the universe's fundamental properties.

Scientists have known for almost a century that the universe is expanding, meaning the distance between galaxies across the universe is becoming ever more vast every second. But exactly how fast space is stretching, a value known as the Hubble constant, has remained stubbornly elusive.

Now, University of Chicago professor Wendy Freedman and colleagues have a new measurement for the rate of expansion in the modern universe, suggesting the space between galaxies is stretching faster than scientists would expect. Freedman's is one of several recent studies that point to a nagging discrepancy between modern expansion measurements and predictions based on the universe as it was more than 13 billion years ago, as measured by the European Space Agency's Planck satellite.

As more research points to a discrepancy between predictions and observations, scientists are considering whether they may need to come up with a new model for the underlying physics of the universe in order to explain it.

"The Hubble constant is the cosmological parameter that sets the absolute scale, size and age of the universe; it is one of the most direct ways we have of quantifying how the universe evolves," said Freedman. "The discrepancy that we saw before has not gone away, but this new evidence suggests that the jury is still out on whether there is an immediate and compelling reason to believe that there is something fundamentally flawed in our current model of the universe."

In a new paper accepted for publication in The Astrophysical Journal, Freedman and her team announced a new measurement of the Hubble constant using a kind of star known as a red giant. Their new observations, made using Hubble, indicate that the expansion rate for the nearby universe is just under 70 kilometers per second per megaparsec (km/sec/Mpc). One parsec is equivalent to 3.26 light-years distance.

This measurement is slightly smaller than the value of 74 km/sec/Mpc recently reported by the Hubble SH0ES (Supernovae H0 for the Equation of State) team using Cepheid variables, which are stars that pulse at regular intervals that correspond to their peak brightness. This team, led by Adam Riess of the Johns Hopkins University and Space Telescope Science Institute, Baltimore, Maryland, recently reported refining their observations to the highest precision to date for their Cepheid distance measurement technique.

How to Measure Expansion

A central challenge in measuring the universe's expansion rate is that it is very difficult to accurately calculate distances to distant objects.

In 2001, Freedman led a team that used distant stars to make a landmark measurement of the Hubble constant. The Hubble Space Telescope Key Project team measured the value using Cepheid variables as distance markers. Their program concluded that the value of the Hubble constant for our universe was 72 km/sec/Mpc.

But more recently, scientists took a very different approach: building a model based on the rippling structure of light left over from the big bang, which is called the Cosmic Microwave Background. The Planck measurements allow scientists to predict how the early universe would likely have evolved into the expansion rate astronomers can measure today. Scientists calculated a value of 67.4 km/sec/Mpc, in significant disagreement with the rate of 74.0 km/sec/Mpc measured with Cepheid stars.

Astronomers have looked for anything that might be causing the mismatch. "Naturally, questions arise as to whether the discrepancy is coming from some aspect that astronomers don't yet understand about the stars we're measuring, or whether our cosmological model of the universe is still incomplete," Freedman said. "Or maybe both need to be improved upon."

Freedman's team sought to check their results by establishing a new and entirely independent path to the Hubble constant using an entirely different kind of star.

Certain stars end their lives as a very luminous kind of star called a red giant, a stage of evolution that our own Sun will experience billions of years from now. At a certain point, the star undergoes a catastrophic event called a helium flash, in which the temperature rises to about 100 million degrees and the structure of the star is rearranged, which ultimately dramatically decreases its luminosity. Astronomers can measure the apparent brightness of the red giant stars at this stage in different galaxies, and they can use this as a way to tell their distance.

The Hubble constant is calculated by comparing distance values to the apparent recessional velocity of the target galaxies—that is, how fast galaxies seem to be moving away. The team's calculations give a Hubble constant of 69.8 km/sec/Mpc—straddling the values derived by the Planck and Riess teams.

"Our initial thought was that if there's a problem to be resolved between the Cepheids and the Cosmic Microwave Background, then the red giant method can be the tie-breaker," said Freedman.

But the results do not appear to strongly favor one answer over the other say the researchers, although they align more closely with the Planck results.

NASA's upcoming mission, the Wide Field Infrared Survey Telescope (WFIRST), scheduled to launch in the mid-2020s, will enable astronomers to better explore the value of the Hubble constant across cosmic time. WFIRST, with its Hubble-like resolution and 100 times greater view of the sky, will provide a wealth of new Type Ia supernovae, Cepheid variables, and red giant stars to fundamentally improve distance measurements to galaxies near and far.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.


TOPICS: Astronomy; History; Science; UFO's
KEYWORDS: astronomy; haltonarp; hubbleconstant; hubbleinconstant; kludge; savethetheory; science; stringtheory
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1 posted on 07/16/2019 10:11:43 AM PDT by Red Badger
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To: SunkenCiv

PinGGG!....................


2 posted on 07/16/2019 10:12:30 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: Red Badger

Uh, Trump caused galactic warming is causing the rapid expansion. Just ask billy nye. :-)


3 posted on 07/16/2019 10:20:54 AM PDT by rktman ( #My2ndAmend! ----- Enlisted in the Navy in '67 to protect folks rights to strip my rights. WTH?)
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To: Red Badger

So the farther in universe we look, the faster objects appear to be speeding away from each other. But the farther we look, the further back in time we’re looking as well. So does this mean the universe is actually slowing down as it ages - nearer objects are older and not moving apart as fast as distant objects (star/galaxies)?


4 posted on 07/16/2019 10:46:27 AM PDT by amorphous
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To: Red Badger
My personal observations and measurements of the Hubble constant are closer to 77 km/sec/Mpc...

I ignore both Cepheids and red giants and focus entirely on pictures of Chelsea's dad and the expanding size and mass of her mother...

5 posted on 07/16/2019 10:47:06 AM PDT by SuperLuminal (Where is Sam Adams now that we desperately need him)
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To: Red Badger

What if I told you our “constants” aren’t constant? Would your dogma force you to balk?


6 posted on 07/16/2019 10:51:59 AM PDT by numberonepal (WWG1WGA)
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To: Red Badger
Dark Matter.

Everything in cosmetology can be explained by invoking Dark Matter.

It's the universal fudge-factor.

7 posted on 07/16/2019 11:00:48 AM PDT by yesthatjallen
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To: amorphous

1. The Universe was smaller way back then.

2. Light was faster way back then................


8 posted on 07/16/2019 11:01:36 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: numberonepal

The only constant is change...............


9 posted on 07/16/2019 11:02:23 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: Red Badger

If the Universe is expanding (Yes, I know it’s trying
to get away from Chuck Norris.) then the distance between
atomic particles must be increasing also...?

Probably harder to measure though.


10 posted on 07/16/2019 11:08:10 AM PDT by tet68 ( " We would not die in that man's company, that fears his fellowship to die with us...." Henry V.)
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To: tet68

that should follow, that if ‘space’ itself is expanding, the the ‘space’ between atomic particles is as well..............


11 posted on 07/16/2019 11:20:41 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: yesthatjallen

I don’t know, therefore, Dark Matter.........


12 posted on 07/16/2019 11:21:17 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: Red Badger
The only constant is change...

Always hopeful yet discontent
He knows changes aren't permanent
But change is.

13 posted on 07/16/2019 11:25:34 AM PDT by Bloody Sam Roberts (Elitist Liberals have no idea the hunger and strength of the beast they have uncaged.)
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To: Red Badger

So, the whole equation is based on the “fact” that they observed “how many”(?) red giants over the lifetime of the star and determined “when” in that life cycle they peak ( and they all peaked at the same age). The whole equation is based on some obscure assumption not observable by anyone, certainly not a population of RGs and not even one. ( they burn for how long again?)


14 posted on 07/16/2019 11:29:05 AM PDT by Manly Warrior (US ARMY (Ret), "No Free Lunches for the Dogs of War")
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To: Red Badger
None of your points answer my question.

On your second point, 2. Light was faster way back then................, would imply a medium exists which affects the speed of light which violates Einstein's long established relativity theory - no?

On your first point, 1. The Universe was smaller way back then. What if the universe was actually larger back then? What if instead of expanding, the universe is actually contracting, growing smaller at an ever increasing rate like expanding foam, but in reverse?

15 posted on 07/16/2019 11:34:37 AM PDT by amorphous
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To: amorphous

Einstein’s Speed of light limitation is good only within its frame of reference.

As the universe expands, the speed of light as observed from a great distance appears to slow down, but within that frame of reference the speed of light never changes..........


16 posted on 07/16/2019 11:37:33 AM PDT by Red Badger (We are headed for a Civil War. It won't be nice like the last one....................)
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To: amorphous
What if instead of expanding, the universe is actually contracting, growing smaller at an ever increasing rate like expanding foam, but in reverse?

The Universe is a gigantic Black Hole. All galaxies are "falling" down the hole.

Galaxies "farther down" the hole are "falling" faster than us and appear to be receding from us.

Galaxies for which we are "farther" down are not "falling" as fast as we and also appear to be receding from us.

I wish I had the Math capability to examine this theory.

17 posted on 07/16/2019 11:51:45 AM PDT by eCSMaster ( The following statement is false. The previous statement is true.)
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To: eCSMaster

The “Big Bang” is the Event Horizon for this Black Hole.


18 posted on 07/16/2019 11:56:01 AM PDT by eCSMaster ( The following statement is false. The previous statement is true.)
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To: eCSMaster

If that was the case shouldn’t there be some galaxies
that appear to be stationary, ie falling at the same
rate as ourselves, unless once you enter a black hole
everything starts expanding again???

Signed Confused.

Ps. While this text appears to me here and now it’s
actually there and then to you. Quantum textual entanglement?


19 posted on 07/16/2019 11:58:24 AM PDT by tet68 ( " We would not die in that man's company, that fears his fellowship to die with us...." Henry V.)
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To: amorphous

So the farther in universe we look, the faster objects appear to be speeding away from each other. But the farther we look, the further back in time we’re looking as well. So does this mean the universe is actually slowing down as it ages - nearer objects are older and not moving apart as fast as distant objects (star/galaxies)?
+++++
You have a point.

But remember, it is space that is expanding.

I tend to think of space as a giant balloon that is being blown up. If you are a particle near the center of that balloon you would hardly notice. But if you are closer to the balloon itself your wiggle room would be getting increasingly more comfortable.

It’s a 4/3 PI R3 thing. And although we are not likely to be at the center of the universe our ability to look at that universe is limited to something like 13.8 billion light years in any direction. That’s what we can see. And it is a sphere inside a much bigger universe.

Don’t use any of this to answer questions on your next physics test. It is simply my imagination going crazy with only a fact or two as backup.


20 posted on 07/16/2019 12:33:01 PM PDT by InterceptPoint (Ted, you finally endorsed. A)
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