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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 .
The sizes are listed in units of Jupiter radii (R J, 71 492 km).This list is designed to include all planets that are larger than 1.6 times the size of Jupiter.Some well-known planets that are smaller than 1.6 R J (17.93 R 🜨 or 114 387.2 km) have been included for the sake of comparison.
The planet is calculated to have an accretion rate up to 10 −8 M ☉ per year assuming a planetary mass of 15 M Jup, which would correspond to a planetary radius of 0.13 R ☉ based on evolutionary tracks. [18] Thus, HD 100546 c is either in a relatively quiescent stage or its growth from accretion is at a low level or has already ceased. [18]
The NFL franchise tag's value is dependent on the type of tag and the player's position. Here's what the franchise tag is worth in 2025.
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Exoplanets have been discovered using several different methods for collecting or combining direct images to isolate planets from the background light of their star. Non-Redundant Aperture Masking Interferometry is a method of combining the views of multiple telescopes into a single image, while the other methods are algorithms for combining ...
This dazzling collection of diamond rings was worth a whopping $50,000 (about $654,782 after adjusting for inflation in today’s economy). We bet security was tight during that photoshoot.
ROXs 12b: 16 210 imaging 390 0.87 3850 [61] ROXs 42Bb: 9 157 imaging 440 1 [61] WASP-8c: 9.45 4323 5.28 radial vel. 280 1.03 5600 [62] WASP-65b: 1.55 1.112 2.3114243 0.0334 transit 1000 0.93 5600 [63] WASP-68b: 0.95 1.24 5.084298 0.06206 transit 962 ± 8 1.24 5911 [64] WASP-69b: 0.26 1.057 3.8681382 0.04525 963 transit 160 0.83 4715 [65] WASP ...