![]() |
Exoplanet Discoveries and Updates - Printable Version +- The Orion's Arm Universe Project Forums (https://www.orionsarm.com/forum) +-- Forum: Offtopics and Extras; Other Cool Stuff (https://www.orionsarm.com/forum/forumdisplay.php?fid=2) +--- Forum: Real Life But OA Relevant (https://www.orionsarm.com/forum/forumdisplay.php?fid=7) +--- Thread: Exoplanet Discoveries and Updates (/showthread.php?tid=4240) |
RE: Exoplanet Discoveries and Updates - AstroChara - 04-29-2020 (04-29-2020, 08:37 PM)QuantumJack1 Wrote: I have examined all pages under topic Inner Sphere and found 5 problematic systems requiring edition. Pi Mensae: No problem here, just add planet c. I think we should give the star and its planets some names. Any idea? Gliese 676: I already have some plans for Gliese 676 system. Following the naming convention, the star and the planets can be named Alighieri (star A), Lucifer (Ad), Saint Lucy (Ae), (Dante is located here), Beatrice (Ab), and Virgil (Ac). The companion star could be Boccaccio. Alpha Arietis (Hamal): I think we should do away with the terraformed planet, and the name Gatewai can be applied to the gas giant. Gliese 581: Link to debate. Nu2 Lupi: We can certainly add mentions of them, but they have already been disassembled. RE: Exoplanet Discoveries and Updates - QuantumJack1 - 04-30-2020 8 planetary systems within 15 ly are still blank in EG. These system can be offered to various creative editors for next step worldbuilding. List: Groombridge 34 Ab: 3.03m, 0.072au, T+ Acidian Cytherian; Ac: 36m, 5.4au, N0 Cryoazurian; Gliese 1061 b: 1.38m, 0.021au, T0 Acidian Cytherian; c: 1.75m, 0.035au, T0 Aquean Gaian; d: 1.68m, 0.054au, T0 Aquean Europan; YZ Ceti e: 0.472m, 0.01018au, T0 Mesoazurian Hermian; b: 0.75m, 0.01557au, T0 Mesoazurian Agonian; c: 0.98m, 0.02090au, T0 Acidian Cytherian; d: 1.14m, 0.02764au, T0 Acidian Cytherian; Teegarden's star b: 1.05m, 0.0252au, T0 Aquean Gaian; c: 1.11m, 0.0443au, T0 Aquean Europan; Wolf 1061 b: 1.91m, 0.0375au, T0 Mesoazurian Cytherian; c: 3.41m, 0.0890au, T+ Aquean Gaian; d: 7.7m, 0.470au, N- Ammonian; L 1159-16 b: 4.0m, 0.016au, T+ Acidian Cytherian; c: 26.0m, 0.406au, N0 Methanean; d: 81.5m, 0.881au, J- Cryoazurian; Gliese 674 b: 11.8m, 0.039au, N0 Mesoazurian; Gliese 687 b: 18.394m, 0.16353au, N0 Aquean; RE: Exoplanet Discoveries and Updates - Drashner1 - 04-30-2020 At least some of these may be on the Master Star List - Groombridge 34 is, I don't have time to check the others. If they are not, they can be added. Todd RE: Exoplanet Discoveries and Updates - AstroChara - 04-30-2020 (04-30-2020, 11:02 PM)Drashner1 Wrote: At least some of these may be on the Master Star List - Groombridge 34 is, I don't have time to check the others. If they are not, they can be added. The Groombridge 34 system is being worked on right now, by the way. Feel free to write up one of the other systems. RE: Exoplanet Discoveries and Updates - stevebowers - 05-05-2020 Dagon seems to have evaporated, despite having received an IAU name relatively recently. It was probably a debris cloud caused by a collision. I wouldn't rule out an eventual coalescence, however. https://en.wikipedia.org/wiki/Fomalhaut_b RE: Exoplanet Discoveries and Updates - AstroChara - 05-24-2020 A few days ago, I found a paper measuring 82 Eridani's debris disk's inclination, yielding a result of 50 degrees. Assuming that the planets are aligned with this disk, which is likely, this would mean the known planets in this system would actually be roughly 31% more massive than their minimum mass. Here are the 82 Eridani's planets' true mass (in Earth masses) based on the inclination of the debris disk (also with correct designations, in order of distance from primary): f: 1.34 (likely rocky) b: 3.68 (likely volatile-rich) g: 3.29 (likely volatile-rich) c: 4.60 (likely volatile-rich) d: 6.23 (likely gas-rich) e: 13.39 (Neptunian) Terranova should still be a Mars-size world. The paper also looks at HD 38858, 50 light-years away from Sol, whose sole known planet's minimum mass is twice Neptune's mass and orbit in a moderately eccentric path at roughly 1 AU. RE: Exoplanet Discoveries and Updates - AstroChara - 05-26-2020 New, low-noise RV measurements of Proxima, home to two known planets, has been obtained from the ESPRESSO spectrograph, confirming the presence of Proxima b as well as detecting a second signal with a period of 5.15 days and semi-amplitude of 40 cm/s. If the signal is caused by a planet companion, the signal would correspond to a planet with a minimum mass of 0.29 Earths and a semi-major axis of 0.029 AU. (LINK) Proxima's third planet candidate Semi-major axis: 0.029 AU (calculated by myself, using 0.1221 solar masses for star mass) Orbital period: 5.15 days Minimum mass: 0.29 Earth masses Mass (assuming the same inclination as Proxima c's): 0.62 Earth masses The paper also revised Proxima b's mass, yielding a minimum mass of 1.173 Earth masses. Including inclination (again, assuming the same inclination as c), Proxima b's likely true mass is roughly 2.5 Earth masses. RE: Exoplanet Discoveries and Updates - AstroChara - 06-03-2020 Yet another super-Earth has been found in a tight orbit around the red dwarf star CD Ceti / GJ 1057, 28 light-years away from Sol. (LINK) CD Ceti b Semi-major axis: 0.0185 AU Orbital period: 2.29070 days Minimum mass: 3.95 Earth masses RE: Exoplanet Discoveries and Updates - stevebowers - 06-06-2020 (04-21-2020, 10:59 AM)The Astronomer Wrote: The HST was finally pointed back to Fomalhaut, again confirming that Fomalhaut b is, indeed, a dust cloud created by a collision between two large planetesimals, not a planet. I've simply removed all mention of Dagon from the Fomalhaut article; maybe we can put it back if the name is reused. https://www.orionsarm.com/eg-topic/45cbd30e46c61 RE: Exoplanet Discoveries and Updates - AstroChara - 06-26-2020 The young hot Neptune planet AU Microscopii b has been confirmed. There was news of the planet's detection floating around for a while so I'm not surprised to see it confirmed. They have also detected a single transit of what appears to be the second planet orbiting once every roughly 30 days. This candidate transit corresponds to a planet roughly three-fifth Neptune's radius. AU Microscopii b Semi-major axis: 0.066 AU Eccentricity: 0.10 Orbital period: 8.46321 days Mass: <3.4 Neptunes Radius: 1.08 Neptunes Second AU Microscopii planet candidate Semi-major axis: ~0.15 AU Eccentricity: ~0.20 Orbital period: ~30 days Radius: 0.60 Neptunes |