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宮田隆志研究室
Showing the original Japanese · View translation
中間赤外線の観測装置を自分たちで作り、宇宙のダストを調べる研究室。
AboutAbout the lab
自分の作った装置で、だれも見たことがない宇宙を。
宮田研究室は、
中間赤外線は
観測装置の
地上の
Key terms
- 中間赤外線
- 目に
見える 光より 波長が 長い、 波長3〜 50ミクロンほどの光。 低い 温度の 物質が 出す - ダスト
- 宇宙を
漂う、 ちりのような 固体の 小さな粒。 惑星の 原材料に なる - 原始惑星系円盤
- 生まれたての
星の まわりを 取り巻く ガスと ちりの 円盤。 やがて 惑星が できる 場所 - モニタ観測
- 同じ天体を
くり返し観測し、 明る さなどが 時間とともに どう 変わるかを 記録する 観測
ResearchResearch themes
地上望遠鏡に
*Illustrative imageダストでたどる惑星の誕生
ダストは
*Illustrative imageTAO望遠鏡用の観測装置
東京大学が
*Illustrative image中間赤外線で時間の変化を追う
中間赤外線では
MembersFaculty
宮田研究室の
- Professor宮田 隆志Publications ↗
- Assistant Professor上塚 貴史
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Wolf-Rayet 140 (Webb-MIRI)” NASA/ESA/CSA/STScl/JPL-Caltech / Public domain (cropped)
- ダストで
たどる 惑星の 誕生: “Porous chondriteIDP” The original uploader was Amara at English Wikipedia. / CC BY 1.0 (cropped) - TAO望遠鏡用の
観測装置: “Tokyo Atacama Observatory 3D” Takanori Uchida, Ryo Araya / CC BY 4.0 (cropped) - 中間赤外線で
時間の 変化を 追う : “Cassiopeia A infrared echo (complete)” Meli thev / CC BY-SA 4.0 (cropped) - Related lab (本原顕太郎研究室): “Hubble-ultra-deep-field-20091208-WFC3-IR-full” NASA / Public domain (cropped)
- Related lab (酒向重行研究室): “The Test-Bed Telescope 2 dome at night (eso2107h)” F. Ocaña/J. Isabel/Quasar SR / CC BY 4.0 (cropped)
- Related lab (嶋作研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
- Related lab (Kwon研究室): “Cat's Paw Nebula (NGC 6334)” ESO/J. Emerson/VISTA / CC BY 4.0 (cropped)
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