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>