Question

In: Physics

Explain in detail what our cosmic address is in terms of the structures of the Universe,...

Explain in detail what our cosmic address is in terms of the structures of the Universe, from the objects of the Milky Way to superclusters. NOTE: This is an extended essay question, worth 40 points. The response should be formatted in multi-paragraph essay with attention to essay structure, grammar mechanics, and APA formatting.

Solutions

Expert Solution

Earth's new address: 'Solar System, Milky Way

The supercluster of galaxies that includes the Milky Way is 100 times bigger in volume and mass than previously thought, a team of astronomers says. They have mapped the enormous region and given it the name Laniakea — Hawaiian for 'immeasurable heaven'.

Galaxies tend to huddle in groups called clusters; regions where these clusters are densely packed are known as superclusters. But the definition of these massive cosmic structures is vague.

The new study, published in Nature1, describes a novel way to define where one supercluster ends and another begins. A team led by Brent Tully, an astronomer at the University of Hawaii in Honolulu, charted the motions of galaxies to infer the gravitational landscape of the local Universe, and redraw its map.

Cosmic speed

The team used a database2 that compiles the velocities of 8,000 galaxies, calculated after subtracting the average rate of cosmic expansion. “All these deviations are due to the gravitational pull galaxies feel around them, which comes from mass,” says Tully. The researchers used an algorithm to translate these velocities into a three-dimensional field of galaxy flow and density. “We really can’t claim to have a good understanding of cosmology if we cannot explain this motion,” says Tully.

This method is superior to merely mapping the location of matter, because it enables scientists to build a map of uncharted regions of the Universe, says Paulo Lopes, an astrophysicist at the Valongo Observatory, part of the Federal University of Rio de Janeiro. It relies on detecting the galaxies' influence, rather than seeing them directly.

Moreover, the galaxies' motions reflect the distribution of all matter, not just that which is visible in our telescopes — including dark matter.

Discounting cosmic expansion, their map shows flow lines down which galaxies creep under the effect of gravity in their local region (see video). Based on this, the team defines the edge of a supercluster as the boundary at which these flow lines diverge. On one side of the line, galaxies flow towards one gravitational centre; beyond it, they flow towards another. “It’s like water dividing at a watershed, where it flows either to the left or right of a height of land,” says Tully.

Frontiers in space

This is a completely new definition of a supercluster. Scientists previously placed the Milky Way in the Virgo Supercluster, but under Tully and colleagues' definition, this region becomes just an appendage of the much larger Laniakea, which is 160 million parsecs (520 million light years) across and contains the mass of 100 million billion Suns.

However, this work is unlikely to be the final word on what a supercluster is, says Gayoung Chon, an astronomer at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany. Her team works on a different definition, based on superclusters being structures that will one day collapse into a single object. This will not happen to Laniakea, she estimates, because some of the galaxies within it will recede from one another forever. “The definition you use really depends on the questions you want to ask. This latest method is a very good way to chart the large-scale structures of the Universe, but it doesn’t ask what will happen to these superclusters eventually,” she says.

Although the map is comprehensive over the Universe around the Milky Way, its distance measurements become less accurate, and less numerous, the farther out you go, says Lopes. This is currently the technique’s biggest potential source of error, he says, but adding more galaxy measurements will improve the map and could eventually help scientists to fully trace what is behind the motion of our local group of galaxies.

Earth - 12,700 klick in diameter - Our home planet

Solar System - a pair of light-years across - Our home planetary system. At this time, the Sun's gravity offersthanks to that of encompassing stars.

Local heavenly body Cloud - thirty light-years across - heavenly body cloud of gas through that the Sun and variety of alternative stars square measure presently traveling.

Milky Way Galaxy - a hundred,000 light-years across - Our home galaxy, composed of two hundred billion to four hundred billion stars and stuffed with the interstellar space.

Local Galactic cluster - three megaparsecs across - cluster of a minimum of forty seven galaxies. Dominated by Andromeda (the largest), The Milky Way and Triangulum; the rest square measure tiny dwarf galaxies.

Virgo Supercluster - thirty three megaparsecs across - The supercluster of that our native cluster may be a part; contains roughly a hundred galaxy teams and clusters.

Local Superclusters - three hundred megaparsecs across - The galaxy filament of that the Virgo Supercluster may be a half.

Observable universe - twenty eightythousand megaparsecs across - The large-scale structure of the universe consists of over a hundred billion galaxies, organized in variant superclusters, galactic filaments, and voids, making a foam-like structure.

Universe - Minimum of twenty eightthousand mega per secs - on the far side the evident universe lies the imperceptible regions wherever no light-weight from those regions has reached the world nonetheless.


Related Solutions

Inflation (a) What is the cosmic epoch of inflation in the early universe? How is this...
Inflation (a) What is the cosmic epoch of inflation in the early universe? How is this different from the usual expansion of the universe? (b) What similarities and differences are there between inflation and dark energy?
Cosmic Contraptions (a) The Friedmann equations describing our universe at large scales are 12(??(?)??)2−4???(?)3?2(?)=−??22ℓ2 and ???(?(?)?3(?))=−?(?)????3(?)...
Cosmic Contraptions (a) The Friedmann equations describing our universe at large scales are 12(??(?)??)2−4???(?)3?2(?)=−??22ℓ2 and ???(?(?)?3(?))=−?(?)????3(?) for the scale factor ?(?). Explain the meaning of the quantities ?, ℓ, ?, and ? in these equations. (b) Suppose that the scale factor ?(?)=?0?1/2. If ?=0, find the dependence of ? and ? on ?. What cosmic era does this correspond to? (c) A theorist comes up with a theory of dark matter that indicates the equation of state of the dark...
our universe was made by a powerful Intelligence who exists outside our universe, and in whose...
our universe was made by a powerful Intelligence who exists outside our universe, and in whose image we are made. explain, with reference to James Gardner’s Biocosm hypothesis.
Explain in detail why elementary geometry (used in triangulation) is essential for charting the Universe and...
Explain in detail why elementary geometry (used in triangulation) is essential for charting the Universe and measuring distances in astronomy. NOTE: This is an extended essay question, worth 40 points. The response should be formatted in multi-paragraph essay with attention to essay structure, grammar mechanics, and APA formatting.
16. The cosmic microwave background radiation (CMB) is radiation that bathes the Universe from every direction,...
16. The cosmic microwave background radiation (CMB) is radiation that bathes the Universe from every direction, and appears to be emitted by a blackbody at a temperature of 2.7 Kelvins. This radiation a. comes from stars. b. comes from supernovae. c. is the redshifted glow of the hot young universe, appearing much cooler today. d. consists of cosmic rays emitted by dying stars.
Explain the concept of the Production Possibilities Curve. What does it represent in terms of our...
Explain the concept of the Production Possibilities Curve. What does it represent in terms of our Macro economic system? Using your own data, draw a curve which represents the Law of Increasing Opportunity Costs and explain how those costs are considered as Increasing. Explain how the PPF is similar to the Business Cycle concept.
Why was inflation introduced into models of our universe (i.e. What problem did inflation solve?) What...
Why was inflation introduced into models of our universe (i.e. What problem did inflation solve?) What is symmetry breaking and how did it occur in the early universe? What are the four fundamental forces symmetry breaking created? Which of the fundamental forces have physicists explained fully? Which are we still struggling to explain fully? How would the universe differ if inflation never occurred?
Explain in terms of atomic and molecular structures and/or intermolecular forces. The ions of NaF and...
Explain in terms of atomic and molecular structures and/or intermolecular forces. The ions of NaF and MgO are isoelectronic and the interatomic distances are about the same. Yet MgO melts at 2642 C while NaF melts at 992 C.
How does the multiverse solve the problem of our universe being just right for life? What...
How does the multiverse solve the problem of our universe being just right for life? What evidence can you cite (a) in favor of the multiverse, and (b) against the multiverse? Explain briefly each level of Max Tegmark's universe? It has often been argued that the multiverse theory has no merit because it can't be disproved. How do you respond to this critique?
Is every galaxy in the universe rotating in the same way as our solar system?
Is every galaxy in the universe rotating in the same way as our solar system?
ADVERTISEMENT
ADVERTISEMENT
ADVERTISEMENT