<system>
	<name>HIP 63242</name>
	<rightascension>12 57 31.9599</rightascension>
	<declination>-65 38 47.2594</declination>
	<distance>135</distance>
	<star>
		<name>HIP 63242</name>
		<name>Gaia DR2 5858576597131420288</name>
		<name>TYC 9001-513-1</name>
		<name>HD 112410</name>
		<mass errorminus="0.05" errorplus="0.05">1.54</mass>
		<temperature errorminus="100" errorplus="100">4839</temperature>
		<magV errorminus="0.01" errorplus="0.01">6.86</magV>
		<magB errorminus="0.02" errorplus="0.02">7.90</magB>
		<magJ errorminus="0.023" errorplus="0.023">5.045</magJ>
		<magH errorminus="0.027" errorplus="0.027">4.581</magH>
		<magK errorminus="0.016" errorplus="0.016">4.406</magK>
		<metallicity errorminus="0.09" errorplus="0.09">-0.31</metallicity>
		<spectraltype>G8III</spectraltype>
		<planet>
			<name>HIP 63242 b</name>
			<name>Gaia DR2 5858576597131420288 b</name>
			<name>TYC 9001-513-1 b</name>
			<name>HD 112410 b</name>
			<list>Confirmed planets</list>
			<mass>9.18</mass>
			<period>124.6</period>
			<semimajoraxis>0.565</semimajoraxis>
			<eccentricity>0.23</eccentricity>
			<periastron>118.2</periastron>
			<description>The planet HIP 63242 b is the innermost planet detected around any intermediate-mass giant star. The lack of other close-in planets suggests that these planets might be destroyed by the large envelope of the host star during the red giant phase.</description>
			<discoverymethod>RV</discoverymethod>
			<lastupdate>13/06/18</lastupdate>
			<discoveryyear>2013</discoveryyear>
		</planet>
	</star>
	<constellation>Musca</constellation>
</system>
