Colors have been derived from the observed optical spectrum of Mars and Jupiter. It is known that the planets and the Moon emit re ected sunlight and thus their spectra are similar to the spectrum of solar radiation. The question was then why is the color of Mars different from that of other planets, i.e. red, although it would share the same spectrum of re ected sunlight. Can one derive color from the spectrum? Therefore, we observed the optical spectra of the scattered sunlight in day time for the Moon and Mars using a 1-D array spectrograph on the 12-inch reflecting telescope in the Korea Science Academy of KAIST in Busan, Korea. We adopted the International Commission on Illumination (CIE) in 1931 of three spectral sensitivity peaks for the human eye in short, medium and long wavelengths in visible light. The observed spectra were imposed on CIE sensitivities and the color detected by the human eye was derived. The Mars spectrum represents red color and the Moon white. It is a similar color to that which a human would see. This result means that color is easily derived from astronomical spectra. The appearance of the planets surface can be determined for Mars, which is the result of iron oxide.

ABSTRACT
1. INTRODUCTION
2. DATA
3. BOLOMETRIC COLOR
4. RESULTS
5. SUMMARY
REFERENCES

• Seung-A Lee(Korea Science Academy of KAIST)
• Dong-Eun Lee(Korea Science Academy of KAIST)
• Yeung-Hun Jo(Korea Science Academy of KAIST)
• In-Ok Song(Korea Science Academy of KAIST)