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首页> 外文期刊>The Astrophysical Journal. Letters >The deep blue color of HD 189733b: Albedo measurements with Hubble Space Telescope/Space Telescope imaging spectrograph at visible wavelengths
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The deep blue color of HD 189733b: Albedo measurements with Hubble Space Telescope/Space Telescope imaging spectrograph at visible wavelengths

机译:HD 189733b的深蓝色:哈勃太空望远镜/太空望远镜成像光谱仪在可见光波长下的反照率测量

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We present a secondary eclipse observation for the hot Jupiter HD 189733b across the wavelength range 290-570 nm made using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. We measure geometric albedos of A_g = 0.40 ± 0.12 across 290-450 nm and A_g < 0.12 across 450-570 nm at 1σ confidence. The albedo decrease toward longer wavelengths is also apparent when using six wavelength bins over the same wavelength range. This can be interpreted as evidence for optically thick reflective clouds on the dayside hemisphere with sodium absorption suppressing the scattered light signal beyond 450 nm. Our best-fit albedo values imply that HD 189733b would appear a deep blue color at visible wavelengths.
机译:我们在哈勃太空望远镜上使用太空望远镜成像光谱仪在290-570 nm的波长范围内对热木星HD 189733b进行了日食观测。我们以1σ置信度在290-450 nm范围内测量A_g = 0.40±0.12的几何反照率,在450-570 nm范围内测量A_g <0.12的几何反照率。当在相同波长范围内使用六个波长仓时,反照率向更长波长的降低也很明显。这可以解释为白天半球上光学上厚厚的反射云的证据,钠吸收抑制了超过450 nm的散射光信号。我们最适合的反照率值意味着HD 189733b在可见波长下会显示深蓝色。

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