Kilonova

Stsci_2020-48a_1024

stsci_2020-48a January 5th, 2020

Credit: NASA, ESA, STScI, W. Fong (Northwestern)

Long ago and far across the universe, an enormous burst of gamma rays unleashed more energy in a half-second than the Sun will produce over its entire 10-billion-year lifetime. In May of this year, scientists detected the light from that flash as it finally reached Earth. They quickly trained NASA’s Hubble Space Telescope on the location to study the associated afterglow. Based on X-ray and radio observations from other observatories, the team was baffled by what they saw with Hubble — the near-infrared emission detected by Hubble was 10 times brighter than predicted.

These results challenge conventional theories of what happens in the aftermath of a gamma-ray burst. One possibility is that the observations might point to the birth of a massive, highly magnetized neutron star called a magnetar.

“These observations do not fit traditional explanations for short gamma-ray bursts,” said study leader Wen-fai Fong of Northwestern University in Evanston, Illinois. “Given what we know about the radio and X-rays from this blast, it just doesn’t match up. The near-infrared emission that we’re finding with Hubble is way too bright. In terms of trying to fit the puzzle pieces of this gamma-ray burst together, one puzzle piece is not fitting correctly.”

Without Hubble, the gamma-ray burst (GRB) would have appeared like many other GRBs, and Fong and her team would not have known about the bizarre infrared behavior. “It’s amazing to me that after 10 years of studying the same type of phenomenon, that we can discover unprecedented behavior like this,” said Fong. “It just reveals the diversity of explosions that the universe is capable of producing, which is very exciting.”

Light Fantastic

The intense flashes of gamma rays from these bursts appear to come from jets of material that are moving extremely close to the speed of light. The jets do not contain a lot of mass — maybe a millionth of the mass of the Sun — but because they’re moving so fast

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2020/news-2020-48

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

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Image Details Image Details

Image Type
Observation
Object Name
GRB 2005-22A
Subject - Distant Universe
Cosmology > Phenomenon > Gamma Ray Burst
Star > Evolutionary Stage > Neutron Star

Distance Details Distance

Universescale3
5,440,000,000 light years

Position Details Position Details

Position (ICRS)
RA = 0h 22m 43.7s
DEC = 0° 16’ 59.4”
Constellation
Pisces

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Orange Hubble (WFC3) Infrared (J) 1.3 µm
Cyan Hubble (WFC3) Infrared (H) 1.5 µm
Spectrum_base
Orange
Cyan
Stsci_2020-48a_1280
×
ID
2020-48a
Subject Category
D.6.2.2   D.3.1.9  
Subject Name
GRB 2005-22A
Credits
NASA, ESA, STScI, W. Fong (Northwestern)
Release Date
2020-01-05T00:00:00
Lightyears
5,440,000,000
Redshift
5,440,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2020/news-2020-48
Type
Observation
Image Quality
Good
Distance Notes
Distance in Lightyears
Facility
Hubble, Hubble
Instrument
WFC3, WFC3
Color Assignment
Orange, Cyan
Band
Infrared, Infrared
Bandpass
J, H
Central Wavelength
1250, 1500
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
Reference Value
5.682, -0.28316667
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
Position
FITS Header
Notes
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p2048a-f-608x608.tif
Metadata Date
2021-12-14T13:44:33-05:00
Metadata Version
1.2
×

 

Detailed color mapping information coming soon...

×
Universescalefull
5,440,000,000 light years

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