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Bibiana Prinoth<p>They observed WASP-12 b 45 times with <a href="https://astrodon.social/tags/CHEOPS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>CHEOPS</span></a> and used <a href="https://astrodon.social/tags/TESS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>TESS</span></a> and <a href="https://astrodon.social/tags/Spitzer" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>Spitzer</span></a> data to study the phase curve including tidal deformation. </p><p>Why is tidal deformation important? If you don’t account for the shape, you’ll overestimate the density of your planet. </p><p>The phase curves allow to calculate the Love number which should tell us about the core mass fraction. Sadly not very well constrained, so we need <a href="https://astrodon.social/tags/JWST" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>JWST</span></a> for that instead. They’ll be doing that for WASP-103 b. </p><p><a href="https://astrodon.social/tags/ExSSV" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>ExSSV</span></a></p>
Bibiana Prinoth<p>We continue with David Ehrenreich on the v² Lupi system: a tale of three sub-Neptunian worlds in the evaporation valley. </p><p>Close-in sub-Neptune planets experience mass loss, also young ones and it could be the reason for the observed radius value. So there is a high interest in studying cooler longer period sub-Neptunes.</p><p>This leads to the synergy of CHEOPS and TESS 🙌🏻 <a href="https://astrodon.social/tags/TESS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>TESS</span></a> finds, <a href="https://astrodon.social/tags/CHEOPS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>CHEOPS</span></a> follows up. <a href="https://astrodon.social/tags/ExSSV" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>ExSSV</span></a></p>
Matt Willemsen<p>Cosmic Symphony: Cheops Mission Exposes a Resonant Sextet of Distant Worlds<br><a href="https://scitechdaily.com/cosmic-symphony-cheops-mission-exposes-a-resonant-sextet-of-distant-worlds/" rel="nofollow noopener noreferrer" translate="no" target="_blank"><span class="invisible">https://</span><span class="ellipsis">scitechdaily.com/cosmic-sympho</span><span class="invisible">ny-cheops-mission-exposes-a-resonant-sextet-of-distant-worlds/</span></a> <a href="https://mastodon.social/tags/CHEOPS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>CHEOPS</span></a> <a href="https://mastodon.social/tags/exoplanets" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>exoplanets</span></a> <a href="https://mastodon.social/tags/resonant" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>resonant</span></a> <a href="https://mastodon.social/tags/ComaBerenices" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>ComaBerenices</span></a> <a href="https://mastodon.social/tags/TESS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>TESS</span></a></p>
The European Network<p>A European spacecraft has revealed the secrets of a star system that has puzzled researchers for years.</p><p>The rare six sextuplet of planets was found thanks to data collected by Cheops — the CHaracterising ExOPlanets Satellite.</p><p>Cheops is a European Space Agency (ESA) mission to study known exoplanets, which are any planets beyond our solar system. Its latest discovery emerged from confusion surrounding a star called HD110067.</p><p><a href="https://thenextweb.com/news/esa-cheops-spacecraft-discovers-star-system" rel="nofollow noopener noreferrer" translate="no" target="_blank"><span class="invisible">https://</span><span class="ellipsis">thenextweb.com/news/esa-cheops</span><span class="invisible">-spacecraft-discovers-star-system</span></a></p><p><a href="https://mstdn.social/tags/ESA" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>ESA</span></a> <a href="https://mstdn.social/tags/Space" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>Space</span></a> <a href="https://mstdn.social/tags/Planet" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>Planet</span></a> <a href="https://mstdn.social/tags/Satellite" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>Satellite</span></a> <a href="https://mstdn.social/tags/CHEOPS" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>CHEOPS</span></a></p>
Mikko Tuomi<p>Data from the exoplanet mission <a href="https://scicomm.xyz/tags/Cheops" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>Cheops</span></a> has led to the surprising revelation that an ultra-hot <a href="https://scicomm.xyz/tags/exoplanet" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>exoplanet</span></a> that orbits its host star in less than a day is covered by reflective clouds of metal, making it the shiniest exoplanet ever found.</p><p>LTT9779&nbsp;b’s high albedo came as a surprise because the planet’s side facing its star is estimated to be around 2000&nbsp;°C.</p><p>No other <a href="https://scicomm.xyz/tags/planets" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>planets</span></a> of this size and mass have been found to orbit so close to their <a href="https://scicomm.xyz/tags/star" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>star</span></a>.</p><p><a href="https://scicomm.xyz/tags/exoplanets" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>exoplanets</span></a> <a href="https://scicomm.xyz/tags/astronomy" class="mention hashtag" rel="nofollow noopener noreferrer" target="_blank">#<span>astronomy</span></a><br><a href="https://www.esa.int/Science_Exploration/Space_Science/Cheops/Cheops_shows_scorching_exoplanet_acts_like_a_mirror" rel="nofollow noopener noreferrer" target="_blank"><span class="invisible">https://www.</span><span class="ellipsis">esa.int/Science_Exploration/Sp</span><span class="invisible">ace_Science/Cheops/Cheops_shows_scorching_exoplanet_acts_like_a_mirror</span></a></p>