Bat Shadow

Stsci_2020-22a_1024

stsci_2020-22a May 21st, 2020

Credit: NASA, ESA, and STScI

Shadows on Earth can be mysterious and foreboding, but when they occur in space, they can convey information we otherwise could not know. In a stellar nursery called the Serpens Nebula, nearly 1,300 light-years away, a young star’s game of shadow play is revealing secrets of its unseen planet-forming disk. The near-infrared vision of NASA’s Hubble Space Telescope captured the shadow cast by the fledgling star’s brilliant light being blocked by this disk. Named HBC 672, this Sun-like star is surrounded by a debris ring of dust, rock, and ice—a disk that is too small and too distant to be seen, even by Hubble. But like a little fly that wanders into the beam of a flashlight shining on a wall, its shadow is projected large upon the cloud in which it was born. In this Hubble image, the feature—nicknamed the “Bat Shadow”—spans approximately 200 times the length of our solar system. It is visible in the upper right portion of the picture. “This is an analog of what the solar system looked like when it was only 1 or 2 million years old,” explained Klaus Pontoppidan, an astronomer at the Space Telescope Science Institute (STScI) in Baltimore, Maryland. “For all we know, the solar system once created a shadow like this.” The presence of a shadow means that the disk is being viewed nearly edge-on. This is something that could not otherwise be known because of the disk’s great distance from us, which makes it too small to be seen by Hubble. The disk’s shadow is similar to what is produced by a cylindrical lamp shade. Light escapes from the top and bottom of the shade, but along its circumference, dark cones of shadow form. Although the disk that gives rise to the shadow is a common object around young stars, the combination of an edge-on viewing angle and the surrounding nebula is rare. Scientists can use the shadow to figure out the shape of the disk. For example, they now know that the disk is puffy, which implies that it is full of gas. While most of the shadow is completely opaque, scientists can look for color differences along its edges, where some light gets through. They can use the shape and color of the shadow to determine the size and composition of dust grains suspended in the disk. “These shadows are not easily seen in visible light, but the stellar disks and the shadows they project onto the surrounding nebula can be easily detected in infrared light,” said Max Mutchler, a research and instrument scientist at STScI. “This infrared Bat Shadow reveals properties of both the small, dusty disk and the much larger nebula.” The shadow is an example of what the future James Webb Space Telescope will be capable of studying in even greater depth. “Webb’s power lies in its ability to see into the dust and gas of these disks to understand the material that comprises these environments that form planets,” explained scientist Alexandra Lockwood of STScI. A similar-looking shadow phenomenon emanates from another young star, at the upper left of the Hubble image. At the lower right, what appears to be a void is likely a part of a foreground cloud. Light from the red, double star inside the “void” is partially blocked by this cloud. The image will be used with NASA’s Universe of Learning to illustrate how shadows can convey information about phenomena invisible to us. This program creates materials and experiences to enable learners to explore the universe for themselves. NASA’s Universe of Learning materials are based upon work supported by NASA under award number NNX16AC65A. The Hubble Space Telescope is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, in Washington, D.C. For more information about NASA’s Universe of Learning, see: https://www.universe-of-learning.org/

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2020/news-2020-22

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
Serpens Nebula EC 82
Subject - Milky Way
Star > Evolutionary Stage > Young Stellar Object
Star > Circumstellar Material > Disk > Protoplanetary
Nebula > Appearance > Reflection

Distance Details Distance

Universescale1
1,300 light years
Stsci_2020-22a_128
 

Position Details Position Details

Position (ICRS)
RA = 18h 29m 58.8s
DEC = 1° 14’ 27.7”
Orientation
North is 12.0° CCW
Field of View
2.2 x 2.0 arcminutes
Constellation
Serpens

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Cyan Hubble (WFC3/IR) Infrared (J) 1.3 µm
Orange Hubble (WFC3/IR) Infrared (FeII) 1.6 µm
Spectrum_base
Cyan
Orange
Stsci_2020-22a_1280
×
ID
2020-22a
Subject Category
B.3.1.2   B.3.7.2.1   B.4.2.2  
Subject Name
Serpens Nebula EC 82
Credits
NASA, ESA, and STScI
Release Date
2020-05-21T00:00:00
Lightyears
1,300
Redshift
1,300
Reference Url
https://hubblesite.org/contents/news-releases/2020/news-2020-22
Type
Observation
Image Quality
Good
Distance Notes
Distance in Lightyears
Facility
Hubble, Hubble
Instrument
WFC3/IR, WFC3/IR
Color Assignment
Cyan, Orange
Band
Infrared, Infrared
Bandpass
J, FeII
Central Wavelength
1250, 1640
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
277.49495994905, 1.24102404081
Reference Dimension
4398.00, 3982.00
Reference Pixel
2236.73475951423, 1976.87203399310
Scale
-0.00000832950, 0.00000832950
Rotation
11.98033616503
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center
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-p2022a-f-4398x3982.tif
Metadata Date
2020-05-21T13:02:40-04:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

×
Universescalefull
1,300 light years

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