Young transiting exoplanets (\(R_p/R_\oplus\) planet orbiting a youngsolar analogue with GRACES on Gemini-North. We measured the Doppler tomographic signal of V1298 Tau c and find a projected obliquity of \(\lambda = 5^\circ \pm 15^\circ\), indicating it is well-aligned. The tomographic signal is only seen in the chromospherically driven core of the Ca II Infrared Triplet (IRT), which may be the result of star-planet interactions. Additionally, we find that excess absorption of H\(\alpha\)decreases smoothly during the transit. While this could be a tentative detection an extended hydrogen atmosphere, we find this variationcan be explained by the presence of starspots with surrounding facular regions. More observations both in- and out-of the transits of V1298 Tau c are required to determine the nature of the Ca II IRT and H\(\alpha\)line variations. An interactive version of this poster can be found here!