Hey! What Are You Looking At?

The High Energy Astrophysics Science Archive Research Center (HEASARC) archives space agencies' data from missions studying electromagnetic radiation from extremely energetic cosmic phenomena (e.g., gravitational wave detections, gamma ray bursts, and supernovae). The Canadian Astronomy Data Center (CADC) is another repository containing missions studying comets, asteroids, and exoplanets among other things. Your challenge is to create a visualization tool that can help people interested in these phenomena to access the data quickly and easily.

Exploring The First Light "Cosmic Microwave Background" With WMAP

Summary

The cosmic microwave background (CMB, CMBR), in Big Bang cosmology, is electromagnetic radiation which is a remnant from an early stage of the universe, also known as "relic radiation". The CMB is faint cosmic background radiation filling all space. It is an important source of data on the early universe because it is the oldest electromagnetic radiation in the universe, dating to the epoch of recombination. To study more about this old electromagnetic radiation, a new age probe was sent to detect and observe the remnant of the great explosion "The Big Bang". The probe is called Wilkinson Microwave Anisotropy probe (WMAP) which was named after a great cosmologist David Wilkinson.

How We Addressed This Challenge

We observed and compiled the data obtained from Wilkinson Microwave Anisotropy probe, to get a brief understanding of Microwave Radiation in the background of the universe.


This study is important because this is the only radiation we know till date which is of the same age as of the universe, i.e 13.81 billion years & hence giving it the name "First Light".

It is important to know more about the cosmos, and to find out how the universe begin, at what temperature did the giant explosion took place, how was the universe in the past and what will be its image in the future, because glow of the first light is present in all directions throughout the universe. It is special because, it is present across the globe too!!


What does it do-The entire sky is a source of microwaves in every direction and its presence can be felt when we deal with modern technology, for example in point-to-point communication links, wireless networks, microwave radio relay networks, radar, satellite and spacecraft communication, medical diathermy and cancer treatment, remote sensing, radio astronomy, particle accelerators, spectroscopy and many more.


How does it work- Microwave radiation or Relic radiation is the part of the electromagnetic spectrum and its wavelength varies from 1mm to 1m and its frequency lies in the band of 300GHz to 300MHz. Heat between a source and a recipient can be transferred in three different ways: conduction, when the two are in direct contact, similar to when you touch a hot glass; convection, when the heat is exchanged by a medium, generally fluid, similar to when hot air contacts colder air; lastly, radiation, when the heat is exchanged by the means of an electromagnetic wave, which requires no medium to spread, for example, the warmth conferred by the sun’s light that travelled millions of miles through void(empty) space. This is the only radiation present in the background of the cosmos which gives us an insight about the initial and present temperature of the universe. As time passes the presence of CMB is declining and the temperature is gradually falling down. According to research when the universe was in a compact stage and all of the microwave radiation was confined within a small space its the initial temperature was 1 billion degrees or 109 K and the present temperature of the universe when the microwave is not confined and spread over a large infinite area is approximately 2.73 kelvins.So, we can say that microwave radiation is helpful in preserving the temperature of the universe.


What do you hope to achieve- After our research we got to know about the temperature cycle of the universe, the source of derivation of several factors and theories like a concrete value of Hubble constant, Baryon Density, Cold Dark Matter Density, Physical Baryon Density, Physical Dark Energy Density, Density Fluctuations, Scalar Spectral Index, Reionization Optical Depth, Curvature of the Universe, Tensor to Scalar Ratio, Running Scalar Spectral Index, the hint how the universe begin and probably how will it end, when will the temperature drop to absolute zero.

How We Developed This Project

This topic was chosen because it was interesting and researching about this topic gave us a brief knowledge and information about the formation, temperature & initial stage of the universe. By researching about this topic we came across several interesting and astonishing facts and figures which gave us the base to start and understand several derivation and constants. It gave rise to several mind twisting thoughts and questions which were fun to solve.

Our approach to developing this project was a hardcore research and combining the 9 years data to form a single output about the Relic Radiation provided by the Wilkinson Microwave Anisotropy Probe (WMAP).

No such coding language was used neither any special hardware or software were used in this project. This project is a research based project which do not indulge the use of any coding language, hardware or software.

No as such major problems were faced during the research work and we obtained very high quality results about the topic. After completing the research and study we were able to understand the concrete value of Hubble constant, Baryon Density, Cold Dark Matter Density, Physical Baryon Density, Physical Dark Energy Density, Density Fluctuations, Scalar Spectral Index, Reionization Optical Depth, Curvature of the Universe, Tensor to Scalar Ratio, Running Scalar Spectral Index, the hint how the universe begin and probably how will it end, when will the temperature drop to absolute zero.

How We Used Space Agency Data in This Project

For reference, we considered the data for our research work from https://map.gsfc.nasa.gov/. We used open data too and combined the data which we obtained from the official website and made an suitable output.

The official data was used in our research work very actively and effectively to finalize the data and make a concrete output with minimum errors.

Project Demo

https://drive.google.com/drive/folders/1S6YRmEjA6DxKMFGggzT6TaiwQ3Kyvza5?usp=sharing

Tags
#WMAP #CMB #Microwave #BIGBANG #Universe #Radiations #UniverseDensity #DavidWilkinson #Cosmology #Astrophysics
Judging
This project was submitted for consideration during the Space Apps Judging process.