Images by Date
Images by Category
Solar System
White Dwarfs
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Galaxy Clusters
Cosmology/Deep Field
Images by Interest
Space Scoop for Kids
Sky Map
Photo Blog
Top Rated Images
Image Handouts
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
Chandra Deep Field South Animations
A Tour of Faint Active Nuclei in Chandra Deep Field South
(Credit: NASA/CXC/A. Hobart)
[Runtime: 02:42]

Quicktime MPEG With closed-captions (at YouTube)

A long-standing question in astrophysics is: how and when did supermassive black holes appear and grow in the early universe? New research using NASA's Chandra X-ray Observatory and the Sloan Digital Sky Survey — called the SDSS — suggests that an answer to this question lies with the intermittent way giant black holes may consume material in the first billion years after the Big Bang.

Astronomers have determined the Big Bang occurred about 13.8 billion years ago and have evidence from the SDSS that supermassive black holes with masses of about a billion times that of the sun existed by about 12.8 billion years ago. This implies that supermassive black holes grew rapidly in the first billion years after the Big Bang. Yet, scientists have struggled to find signs of these growing giant black holes.

To address this conundrum, an all-female team of researchers examined different theoretical models and tested them against optical data from the SDSS and X-ray data from Chandra. Their findings indicate that black hole feeding during this era may turn on abruptly and last for short periods of time, which means this growth may be difficult to spot.

The timing of such growth may be key. The authors' model suggests that 13 billion years ago, about one third of supermassive black holes may have been accreting enough matter to be detectable. Just 200 million years earlier — a veritable blip in cosmic time — the number of potentially detectable black holes is only about 3%. In order to test this idea further, the researchers suggest that surveys with Chandra and future X-ray telescope that look at larger areas of the sky in X-rays are necessary.

A Quick Look at Faint Active Nuclei in Chandra Deep Field South
(Credit: NASA/CXC/A. Hobart)
[Runtime: 01:06]

Scientists would like to learn about the earliest supermassive black holes in the Universe.

Supermassive black holes can contain millions or even billions of times the mass of our Sun.

Astronomers find evidence for these giant black holes about a billion years after the Big Bang.

The question is: how did they get so big so quickly?

An all-female team of astrophysicists using X-ray data from Chandra, optical data, and theoretical models is tackling this question.

They found evidence that the very earliest supermassive black holes in the Universe may have grown in intense and sporadic bursts

This "herky jerky" growth may be the key to understanding the origin of these gigantic black holes.

Return to Chandra Deep Field South (May 31, 2017)