Left: Qϕ image of WRAY 15-1880 obtained
from the SPHERE polarimetric data. The red dot at the center of the image marks
the position of the star; the dashed white circle is the size of the
coronagraph used in this observation. The dotted straight lines mark the major
and minor axes, as obtained by Curone et al. (2025). Right: similar image, but
projected on the disk plane (i = 39.22 deg) and rotated to have the major axis
vertical and the minor axis horizontal. Credit: arXiv (2026). DOI: 10.48550/arxiv.2606.10816
Italian astronomers have used the
Very Large Telescope (VLT) to perform polarimetric observations of the star
WRAY 15-1880 and its young circumstellar disk. Results of the new
observations, presented June 10 on the arXiv preprint server, suggest that
this disk may host a primitive planetary system.
A young star with a disk
Circumstellar disks are accretion
disks orbiting stars, composed of gas, dust, planetesimals, asteroids or
collision fragments. Around the youngest stars, they are the reservoirs of
material out of which planets may form.
At a distance of some 492
light-years from Earth, WRAY 15-1880 (also known as RX J1842.9-3532) is a
solar-type classical T Tau star in the CrA-North subregion of the Corona
Australis (CrA) complex. It has a mass of around 1.24 solar masses and is
estimated to be 2.8 million years old.
Previous observations of WRAY
15-1880 have found that it is surrounded by a pre-transitional circumstellar
disk with a gap, whose mass is estimated to be some 0.01 solar masses. The disk
extends to a distance of 87 AU from the star and has an inclination of
approximately 39.32 degrees.
All eyes on WRAY 15-1880
Due to the relative proximity and
young age of WRAY 15-1880, a team of astronomers led by Elisabetta Rigliaco of
the Astronomical Observatory of Padua in Italy turned its attention to this
star and its disk, hoping to gather valuable data on how planetary systems are
born. For this purpose, the team employed VLT's Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) and analyzed archival data from other
VLT instruments and from the Atacama Large Millimeter/submillimeter Array
(ALMA).
The observations conducted by
Rigliaco's team revealed the presence of a companion object possibly orbiting
WRAY 15-1880. The collected data suggest that this object is a Jupiter-like planet with a mass within the range of 1.7–7.6 Jupiter
masses. The spectrum of this source indicates a T3 spectral type, corresponding
to a temperature of about 1,200 K.
Planet or not?
However, the researchers are
cautious about claiming that there is a planet in the disk of WRAY 15-1880.
They explain that they cannot completely exclude the possibility that the
object imaged in high-contrast imaging results from a combination of emission by a
photosphere with starlight reflected or scattered by dust, or that it may
be—for instance—an artifact due to irregularities in the disk structure.
The authors of the paper added that
the candidate exoplanet of WRAY 15-1880 orbits the star on a very wide and
circular orbit—with an orbital period of about 127 years and semimajor axis of
approximately 25.7 AU.
The scientists concluded that if their discovery is confirmed, WRAY 15-1880 would be one of the most primitive forming planetary systems known to date. Moreover, WRAY 15-1880 would also be added to the short list of stars hosting a disk and planets imaged simultaneously.
by Tomasz
Nowakowski, Phys.org
edited by Stephanie Baum, reviewed by Robert Egan
Source: Young disk around WRAY 15-1880 may contain a primitive planetary system

