Images by Date
Images by Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
Multiwavelength
Sky Map
Constellations
3D Wall
Photo Blog
Top Rated Images
Image Handouts
Desktops
High Res Prints
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Getting Hard Copies
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information
Quasars & Active Galaxies
X-ray Astronomy Field Guide
Quasars & Active Galaxies
Questions and Answers
Quasars & Active Galaxies
Chandra Images
Quasars & Active Galaxies
Normal Galaxies & Starburst Galaxies
Related Podcasts
Tour of RX J1131-1231
Download Image

More Information

More Images
Chandra X-ray Image of NGC 1365
(Credit: NASA/CXC/CfA/INAF/Risaliti)

Animation & Video


Related Images
M87
M87
(05 Oct 06)
Abell 400
Cygnus A
Cygnus A
(06 Nov 00)
NGC 1365:
Chandra Sees Remarkable Eclipse of Black Hole



Credit: X-ray: NASA/CXC/CfA/INAF/Risaliti Optical: ESO/VLT

Chandra observations of the galaxy NGC 1365 have captured a remarkable eclipse of the supermassive black hole at its center. A dense cloud of gas passed in front of the black hole, which blocked high-energy X-rays from material close to the black hole. This serendipitous alignment allowed astronomers to measure the size of the disk of material around the black hole, a relatively tiny structure on galactic scales. The Chandra image (shown in the inset) contains a bright X-ray source in the middle, which reveals the position of the supermassive black hole. An optical view of the galaxy from the European Southern Observatory's Very Large Telescope shows the context of the Chandra data.

NGC 1365 contains a so-called active galactic nucleus, or AGN. Scientists believe that the black hole at the center of the AGN is fed by a steady stream of material, presumably in the form of a disk. Material just about to fall into a black hole should be heated to millions of degrees before passing over the event horizon, or point of no return. The process causes the disk of gas around the central black hole in NGC 1365 to produce copious X-rays, but the structure is much too small to resolve directly with a telescope. However, astronomers were able to measure the disk's size by observing how long it took for the black hole to go in and out of the eclipse. This was revealed during a series of observations of NGC 1365 obtained every two days over a period of two weeks in April 2006. During five of the observations, high-energy X-rays from the central X-ray source were visible, but in the second one -- corresponding to the eclipse -- they were not.

Fast Facts for NGC 1365:
Credit  X-ray: NASA/CXC/CfA/INAF/Risaliti Optical: ESO/VLT
Scale  X-ray: 1.2 arcmin per side; Optical: 6.5 arcmin per side
Category  Quasars & Active Galaxies, Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 03h 33m 36.40s | Dec -36 08' 25.00"
Constellation  Fornax
Observation Dates  6 pointings between April 10-23, 2006
Observation Time  25 hours
Obs. IDs  6868 - 6873
Color Code  X-ray: Purple (0.2-1 keV); Yellow (1-2 keV); Blue (2-7 keV)
Instrument  ACIS
References Risaliti et al. 2007, ApJ, 659, L111
Distance Estimate  About 60 million light years
Release Date  April 12, 2007