Search the World Wide Web for information on a European Space Agency mission called Planck. In what ways is Planck an improvement over the WMAP mission? Has it been launched? If yes, what have scientists learned from Planck? If no, what do they hope plan to learn?

Short Answer

Expert verified
Planck is an improvement over the WMAP mission in several ways, including higher resolution and sensitivity, allowing it to measure the Cosmic Microwave Background (CMB) with unprecedented precision. Yes, it was launched and from it, scientists learned more accurate measurements of the parameters of the cosmos, such as the Hubble constant, the age of the universe, and the quantity of dark matter and dark energy.

Step by step solution

01

Research Step: Understanding the Planck Mission

The first step is to find the official or a trustworthy page that contains accurate information about the Planck Mission. Study it carefully, noting its aim, the technology it uses, and its observed findings.
02

Comparison Step: Planck versus WMAP

Next, look into the details of the WMAP mission. Compare the two missions, focusing on aspects such as the technology used, the depth and clarity of the data, and the period of observation.
03

Understanding Improvements: How Planck Is Better

Based on the comparison drawn in the previous step, identify the improvements or advancements the Planck mission has over the WMAP mission.
04

Launch Status: Confirmation of Planck's Launch

Confirm whether the Planck Mission has been launched by searching for its launch date. It's important to verify the data from a reliable source.
05

Findings: What We've Learned from Planck

If Planck has been launched, look for the scientific discoveries or learnings derived from the data it collected.
06

Expectations: Planck's Potential Offerings

If not yet launched, find out the expected outcomes or potential discoveries from the Planck Mission.

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Most popular questions from this chapter

Describe how astronomers use the cosmic background radiation to determine the geometry of the universe.

(a) For what value of the redshift \(z\) were representative distances between galaxies only \(20 \%\) as large as they are now? (b) Compared to representative distances between galaxies in the present-day universe, how large were such distances at \(z=8\) ? Compared to the density of matter in the present-day universe, what was the density of matter at \(z=8\) ? (c) If dark energy is in the form of a cosmological constant, how does its present-day density compare to the density of dark energy at \(z=2\) ? At \(z=5\) ? Explain your answers.

How does modern cosmology preclude the possibility of either a center or an edge to the universe?

Before the discovery of the cosmic microwave background, it seemed possible that we might be living in a "steady-state universe" with overall properties that do not change with time. The steady-state model, like the Big Bang model, assumes an expanding universe, but does not assume a "creation event." Instead, matter is assumed to be created continuously everywhere in space to ensure that the average density of the universe remains constant. Search the World Wide Web for information about the steady-state theory. Explain why the existence of the cosmic microwave background was a fatal blow to the steady- state theory.

What does it mean to say that the universe is darkenergy-dominated? What happened when the universe changed from being matter-dominated to being darkenergy-dominated?

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