Astronomers using the Subaru Telescope and Hubble Space Telescope have
found that Jupiter's Galilean satellites (Io, Europa, Ganymede, and
Callisto) remain slightly bright (up to one millionth of their normal
state) even when in the Jovian shadow and not directly illuminated by
the Sun (Figure 1).
The effect is particularly pronounced for Ganymede and Callisto. The
finding was made by researchers at Tohoku University, Institute of Space
and Astronautical Science/Japan Aerospace Exploration Agency
(ISAS/JAXA), National Astronomical Observatory of Japan (NAOJ), and
elsewhere.
Figure 1: Images of Ganymede and Callisto while
eclipsed by Jupiter obtained during their eclipse. Top left is Ganymede
observed through Subaru Telescope, top right is Ganymede through Hubble
Space Telescope, bottom left is Callisto from Subaru Telescope,
respectively. Each frame is 4 arcsec x 4 arcsec, and the black circle
indicates the apparent diameter of the object. A short movie linked here
shows the Europa's eclipse as it goes into the shadow of Jupiter. From
the top of the video is Europa, Ganymede, and Jupiter, respectively.
(Credit: NAOJ/JAXA/Tohoku University)
The mechanism of this phenomenon is still under
investigation, but the researchers suggest that indirect forward
scattering of sunlight by hazes in the upper Jovian atmosphere could be
the reason for the illumination. This effect is similar to the one that
causes Earth's moon to look red during a total lunar eclipse.
The type of continuous observations of the Galilean
satellites in eclipse made by the Japanese team also provides a much
better basis for studying the hazes in Jupiter's atmosphere, which are
difficult to study otherwise (Note 1).
In addition, this detailed study method for a planetary atmosphere will
provide new insights about the atmospheres of exoplanets, which are
only beginning to be studied.
Dr. Kohji Tsumura (FRIS, Tohoku University), the PI
on the project, explained that this unexpected finding is really the
outcome of attempts to measure diffuse light from the distant universe.
"It is a serendipitous discovery made as a by-product of a cosmological
study," he said. "It is very interesting that it provides us a new
method to investigate the atmosphere of Jupiter and of exoplanets. I
will keep studying from nearby space (the solar system and exoplanets)
out to the farthest universe through this project."
The research team started its observations using IRCS
and AO188 on Subaru Telescope in February of 2012. The idea was to
detect the diffuse light from the most distant parts of the universe. To
do this, team members planned to use the Galilean satellites in eclipse
as "occulters" to block distant background emissions. This would allow
an extremely accurate separation of the background light from the very
bright foreground radiation from our solar system (known as the zodiacal
light).
The team assumed that the Galilean satellites would
be "dark" while in Jupiter's shadow, and the difference in
brightness[??] between the dark satellite as an occulter and its
surrounding sky would allow the team to determine the still-unknown
level of background emission from the distant universe. Instead, they
found an unexpected surprise: Ganymede and Callisto were still somewhat
"bright" (illuminated) even when eclipsed (relative to the expected
level of near-zero). Their eclipsed luminosity was one millionth of
their un-eclipsed brightness, which is low enough that this phenomenon
has been undetected until now (Figure 2).
Figure 2: Schematic drawing of how to measure the background light. By measuring the difference between the light from the eclipsed satellite and the surrounding sky data, one would obtain the background light information, if the eclipsed satellite is completely dark. It turned out that there is still a faint light reflected off from the satellite during the eclipse. (Credit: NAOJ/JAXA/Tohoku University)
To understand why the Galileans remain
ever-so-slightly bright even when they're in eclipse, the project team
of astronomers and planetary scientists considered several theories
based on their multi-band observational data, including data from
Spitzer Space Telescope. The most plausible is that the Galilean
satellites are still illuminated during eclipse by sunlight that is
scattered by hazes in the Jovian upper atmosphere. By comparison, the
sunlight refracted in the atmosphere does not contribute to the
illumination during the eclipse.
Although Jupiter is a familiar planet, there are many
unresolved issues about its atmosphere. One example is the origin of
the cloud particles composing Jupiter's banded appearance. The cloud
particles are assumed to grow from tiny particles called aerosols or
hazes. Researchers expect that those hazes form somewhere in the upper
part of Jupiter's atmosphere, which is very difficult to observe (Figure 3).
The unexpected discovery of haze-induced brightening of the Galileans
provides a new way to study the mysterious part of Jupiter's atmosphere.
In addition, since astronomers usually observe the planets in our solar
system by reflected sunlight, one of the unique aspects of these new
observations at Jupiter is that observers can precisely measure the
transmitted sunlight through the planetary atmosphere (Note 2).
Figure 3: A schematic image of the model to show that
the Galilean satellites eclipsed in Jovian shadow are illuminated by
scattered sunlight by the haze in the Jovian upper atmosphere. The size
and the distance of the satellites are not to the scale. This process is
similar to one that causes red color of the Earth's Moon during its
total eclipse. (Credit: NAOJ/JAXA/Tohoku University/NASA)
This new method of studying the upper atmosphere of
Jupiter via transmitted sunlight provides a basis for the study of other
planetary systems. Exoplanet discoveries now occur quite regularly and
atmospheres around some of them have been investigated using "transit
observations" (when the exoplanet passes between us and the host star,
resulting in the star becoming slightly dimmer). In such observations,
some characteristics of the exoplanet's atmosphere are revealed as host
starlight passes through it. This is the same situation seen with
Jupiter and its Galilean satellites, and makes studies of transmitted
sunlight of the planets in our solar system essential for comparison.
The observations for this project were very
challenging because the Galilean satellites (while eclipsed) are
extremely faint and they are located next to the incredibly bright disk
of Jupiter. In addition, the eclipses only happen at very specific
times, and Jupiter and the satellites are continuously in motion during
the observations. The complexity of the situation requires the
observation procedure to be much more sophisticated. This new discovery
required thorough preparations by the project team and conscientious
support by the operations staff. (Figure 4)
Figure 4: Three-color (JHK) image of Jupiter and
Ganymede obtained by Subaru Telescope. Because Ganymede moves with
respect to Jupiter during the observations, it appears as three
separately colored dots. Image taken at around 5 am, July 27, 2012 in
Hawaii Time. Blue color is for J band (1.3 micrometer), green is for H
band (1.6 micrometer), and red is for K band (2.2 micrometer),
respectively. (Credit: NAOJ/JAXA/Tohoku University)
The results of this study will be published in The
Astrophysical Journal in its July 10, 2014 issue (Tsumura et al. 2014
arXiv: 1405.5280). This research is supported by Japan Society for the
Promotion of Science, KAKENHI (#24111717, #26800112), and NASA through a
grant from Space Telescope Science Institute and Jet Propulsion
Laboratory in U. S. A.
Notes:
- Observations of Jupiter's upper atmosphere were conducted by the Galileo spacecraft, and by "occultation" of microwaves from field stars or spacecraft located behind Jupiter. However, opportunities to observe these events are rare and limited, thus the observations of the Galilean satellite eclipses are a unique method to study Jupiter's upper atmosphere.
- Transmitted light through the planetary atmosphere was observed by the occultation methods described in (*1) and the Venus transit. However, they are very rare events, too.
Paper information:
To appear in the July 10, 2014 issue of the Astrophysical Journal, Volume 789.
"Near-infrared Brightness of the Galilean Satellites Eclipsed in Jovian Shadow: A New Technique to Investigate Jovian Upper Atmosphere"
K. Tsumura (1,2), K. Arimatsu (2,3), E. Egami (4), Y. Hayano (5), C. Honda (6), J. Kimura (7), K. Kuramoto (8), S. Matsuura (2), Y. Minowa (5), K. Nakajima (9), T. Nakamoto (10), M. Shirahata (2, 11), J. Surace (12), Y. Takahash i(8), and T. Wada (2)
"Near-infrared Brightness of the Galilean Satellites Eclipsed in Jovian Shadow: A New Technique to Investigate Jovian Upper Atmosphere"
K. Tsumura (1,2), K. Arimatsu (2,3), E. Egami (4), Y. Hayano (5), C. Honda (6), J. Kimura (7), K. Kuramoto (8), S. Matsuura (2), Y. Minowa (5), K. Nakajima (9), T. Nakamoto (10), M. Shirahata (2, 11), J. Surace (12), Y. Takahash i(8), and T. Wada (2)
1Frontier Research Institute for Interdisciplinary Science, Tohoku University, Japan
2Department of Space Astronomy and
Astrophysics, Institute of Space and Astronoutical Science, Japan
Aerospace Exploration Agency, Japan
3Department of Astronomy, Graduate School of Science, The University of Tokyo, Japan
4Department of Astronomy, Arizona University, U. S. A.
5Subaru Telescope, National Astronomical Observatory of Japan, U. S. A.
6Research Center for Advanced Information
Science and Technology, Aizu Research Cluster for Space Science, The
University of Aizu, Japan
7Earth-Life Science Institute, Tokyo Institute of Technology, Japan
8Department of Cosmosciences, Graduate School of Science, Hokkaido University, Japan
9Department of Earth and Planetary Sciences, Kyushu University, Japan
10Department of Earth and Planetary Sciences, Graduate School of Science and Engineering, Tokyo Institute of Technology, Japan
11National Astronomical Observatory of Japan, Japan