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ROXs 42Bb is a directly imaged planetary-mass companion [1] to the binary M star ROXs 42B, [4] a likely member of the Rho Ophiuchi cloud complex. The companion was announced/discovered on October 17, 2013, by University of Toronto astronomer Thayne Currie.

Oct 24, 2024 · ROXs 42 B b is a gas giant exoplanet that orbits a M-type star. Its mass is 9 Jupiters, it takes 1968.3 years to complete one orbit of its star, and is 157 AU from its star. Its discovery was announced in 2013.

Oct 17, 2013 · ROXs 42 B b is a direct planetary-mass companion to the binary M star ROXs 42 B, a likely member of the Rho Ophiuchi cloud complex. The companion was announced/discovered on October 17, 2013 by University of Toronto astronomer Thayne Currie.

A First-Look Atmospheric Modeling Study of the Young Directly-Imaged Planet-Mass Companion, ROXs 42Bb

Jan 9, 2014 · An unusual stellar object named ROXs 42Bb may represent a new kind of planets or it may be a very rare planet-mass brown dwarf, according to a group of astronomers from Canada, Germany, Japan and the United States.

Nov 22, 2024 · ROXs 42Bb is the largest planet found in the Universe. It has a mass 9 times that of Jupiter and a radius 1.12 times that of Jupiter. ROXs 42 Bb is 440 light years away from Earth. Because it is located outside the Solar System, it is classified as an exoplanet.

A First-look Atmospheric Modeling Study of the Young Directly Imaged Planet-mass Companion, ROXs 42Bb Currie et al. 2014 | Reference Overview All WISE Data Release

mass estimate. A better determined mass for ROXs 42Bb may also clarify how the companion fits within the context of other imaged planetary-mass companions (Currie et al. 2014). In this paper, we perform a first-look atmospheric model-ing study of ROXs 42Bb. Our analyses combine previously published photometry/spectroscopy with new photometry for

May 8, 2014 · Our analysis of ROXs 42Bb's 1–4 μm photometry and K-band spectrum provides strong evidence that its atmosphere is dusty, with an effective temperature of ∼2000 K. ROXs 42Bb's luminosity of log(L/L ☉) ∼ −3.07 ± 0.07, when compared to evolutionary models, implies a mass of 6–12 M J.

We present near-infrared high-contrast imaging photometry and integral field spectroscopy of ROXs 42B, a binary M0 member of the 1-3 Myr old ρ Ophiuchus star-forming region, from data collected over 7 years.