Epoch J2000 Equinox J2000
|Right ascension||14h 08m 10.15451s|
|Declination||−41° 23′ 52.5766″|
|Apparent magnitude (V)||12|
|U−B color index||0.71|
|B−V color index||1.06|
|Radial velocity (Rv)||3.13 km/s|
|Proper motion (μ)|| RA: -29.661 mas/yr |
Dec.: -23.823 mas/yr
|Parallax (π)||8.8159 ± 0.0405 mas|
|Distance||370 ± 2 ly |
(113.4 ± 0.5 pc)
|Rotational velocity (v sin i)||~10 km/s|
PDS 70 (V1032 Centauri) is a low-mass T Tauri star in the constellation Centaurus. Located approximately 370 light-years from Earth, it has a mass of 0.82 M☉, and is approximately 10 million years old. The star has a protoplanetary disk containing two nascent exoplanets, named PDS 70b and PDS 70c, which have been directly imaged by the European Southern Observatory's Very Large Telescope. PDS 70b was the first confirmed protoplanet to be directly imaged.
The protoplanetary disk around PDS 70 was first hypothesized in 1992 and confirmed in 2006 along with a jet-like structure. The disk has a radius of approximately 140 au. In 2012 a large gap (~65 au) in the disk was discovered, which was thought to be caused by planetary formation.
The gap was later found to have multiple regions: large dust grains were absent out to 80 au, while small dust grains were only absent out to the previously-observed 65 au. There is an asymmetry in the overall shape of the gap; these factors indicate that there are likely multiple planets affecting the shape of the gap and the dust distribution.
In results published in 2018, a planet in the disk, named PDS 70b, was imaged by the Very Large Telescope (VLT). With a mass estimated to be a few times greater than Jupiter, the planet is thought to have a temperature of around 1000 °C and an atmosphere with clouds; its orbit has an approximate radius of 3.22 billion kilometres (21.5 au), taking around 120 years for a revolution. Modelling predicts that the planet has acquired its own accretion disk. The accretion disk was observationally confirmed in 2019.
A second planet, named PDS 70c, was discovered in 2019 using the VLT's MUSE spectrograph. The planet orbits its host star at a distance of 5.31 billion kilometres (35.5 au), further away than PDS 70b. PDS 70c is in a near 1:2 orbital resonance with PDS 70b, meaning that PDS 70c completes nearly one revolution once every time PDS 70b completes nearly two.
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