References
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This project aims to study an exoplanet transit using Mt Kent Observatory's robotic telescope. The star chosen was the 7.7 magnitude HD 189733 in Vulpecula, which has a very hot jupiter in close orbit (HD 189733b). This star is a K dwarf, 63 light years away. RA 20h 00.7m, Dec +22 43'. This transit was originally found by the Geneva Observatory, Switzerland.
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