RW Aur A
Credit: Illustration: NASA/CXC/M.Weiss; X-ray spectrum: NASA/CXC/MIT/H.M.Günther
Credit: Illustration: NASA/CXC/M.Weiss; X-ray spectrum: NASA/CXC/MIT/H.M.Günther
This artist's illustration depicts the destruction of a young planet
or planets, which scientists may have witnessed for the first time using
data from NASA's Chandra X-ray Observatory, as described in our latest press release. If this discovery is confirmed, it would give insight into the processes affecting the survival of infant planets.
RW Aur A is a star about 450 light years
from Earth, making it relatively nearby. Since the 1930s, astronomers
have studied RW Aur A and been curious about why the optical light from
this star changes over time. In recent years, scientists have observed
that this variability has increased, with the star dimming even more and
for longer periods of time.
To investigate this mystery, a team of astronomers used Chandra to get information in the X-ray band of the electromagnetic spectrum.
X-rays are generally emitted by more energetic and hotter phenomena
than their optical light counterparts and can reveal information about
different elements, including iron.
The Chandra data suggest that the most recent dimming event from RW
Aur A was caused by the collision of two "planetesimals" (that is,
infant planetary bodies still in the process of formation), including at
least one object large enough to be a planet.
Because the X-rays come from the hot outer atmosphere of the star,
changes in the X-ray spectrum — the intensity of X-rays measured at
different energies — over these three observations were used to probe
the density and composition of the absorbing material around the star.
The team found that the dips in both optical and X-ray light are
caused by dense gas obscuring the star's light. Also, a Chandra
observation in 2017 showed strong emission from iron atoms, indicating
that the disk contained at least 10 times more iron than in the 2013
observation during a bright period.
The Chandra spectra from the 2013 and 2017 observations are shown in an inset in the graphic. The sharp peak on the right side of the 2017 spectrum is a signature of a large amount of iron.
The researchers propose the excess iron was created when the two
planetesimals collided. If one or both planetary bodies are made partly
of iron, their smash-up could release a large amount of iron into the
star's disk and temporarily obscure its light as the material falls into
the star.
A paper describing these results led by Hans Moritz Guenther (MIT's
Kavli Institute for Astrophysics) appears in the most recent issue of
The Astrophysical Journal and is available online.
The other authors on
the paper are Til Birnstiel (Ludwig-Maximillians-University Munich),
David Huenemoerder (MIT), David Principe (MIT), Christian Schneider
(Hamburger Sternwarte), Scott Wolk (Harvard-Smithsonian Center for
Astrophysics), Franky Dubois (Astrolab IRIS), Ludwig Logiie (Astrolab
IRIS), Steve Rau (Astrolab IRIS), and Siegfried Vanaverbeke (Astrolab
IRIS).
NASA's Marshall Space Flight Center in Huntsville, Alabama,
manages the Chandra program for NASA's Science Mission Directorate in
Washington. The Smithsonian Astrophysical Observatory in Cambridge,
Massachusetts, controls Chandra's science and flight operations.
Fast Facts for RW Aur A:
Category: Normal Stars & Star Clusters, Neutron Stars/X-ray Binaries
Coordinates (J2000): RA 05h 07m 49.5s | Dec 30° 24´ 05.1"
Constellation: Aurigae
Observation Date: 4 pointings from Jan 2013-Jan 2017
Observation Time: 75 hours 33 minutes (3 days 2 hours 33 minutes)
Obs. ID: 14539, 17644, 17764, 19980
Instrument: ACIS
References: Günther, H.M. et al, 2018, AJ. (accepted)
Distance Estimate: About 450 light years
Source: NASA’s Chandra X-ray Observatory
