![]() ![]() Refractory condensates to form, including enstatite and forsterite. Ratios translate to planetary brightness temperatures of $926 \pm 12$ K (NRS1)Īnd $1,122 \pm 10$ K (NRS2), which are low enough for a wide range of Ppm (NRS2) for the dayside hemisphere, and $136 \pm 8$ ppm (NRS1) and $630 \pmġ0$ ppm (NRS2) for the nightside hemisphere. Planet-to-star emission ratios of $3,924 \pm 7$ ppm (NRS1) and $4,924 \pm 9$ suppose in first, rough approximation that both rates were uniform and, with WEGENER, that the time since the. Both planets move eastward, but since the Earth moves faster than Mars in its orbit. This is consistent with the strongest daysideĮmission emanating from eastward of the substellar point. A quick demonstration and explanation of retrograde motion. Harmonic dipole, our light curve fits suggest that the phase curve peaksĬoincide with orbital phases $3.36 \pm 0.11$ deg (NRS1) and $2.66 \pm 0.12$ deg Simple brightness map for the planet described by a low-order spherical Eastward Demo (App 1204020) SteamDB Eastward Demo Install Watch Store Hub Patches 0 Charts App info Packages 3 Depots 5 Configuration Related apps Update history Additional Information Supported Languages SteamDB has been running ad-free since 2012. The baseline flux level of 30 ppm/hr (NRS1) and 10 ppm/hr (NRS2). Light curves exhibit minimal systematics, with approximately linear drifts in ![]() Wavelength ranges of 2.70-3.72 micron and 3.82-5.15 micron, respectively. , -no-tide, -sea-surface, -sea-surface-no-tide. Two broadband light curves generated for the NRS1 and NRS2 detectors, covering WASP-121b, is an ultrahot Jupiter with an orbital period of 30.6 hr. Newly-commissioned observatory for exoplanet climate studies. A few weeks ago Valve approached us to ask if we’d like Eastward to participate in their special game demo event, to which we of course said hell yes. NIRSpec instrument, highlighting the exceptional stability of this Download a PDF of the paper titled A JWST NIRSpec Phase Curve for WASP-121b: Dayside Emission Strongest Eastward of the Substellar Point and Nightside Conditions Conducive to Cloud Formation, by Thomas Mikal-Evans and 12 other authors Download PDF Abstract: We present the first exoplanet phase curve measurement made with the JWST
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