Rossiter–McLaughlin effect

spectroscopic phenomenon observed when either an eclipsing binary's secondary star or an extrasolar planet is seen to transit across the face of the primary or parent star.
Class type of: physical phenomenon Q1763739

Facts

3 properties
🏷️ Also known as
en Rossiter-McLaughlin effect en Rossiter–McLaughlin effect de Rossiter-McLaughlin-Effekt es efecto Rossiter-McLaughlin fi Rossiterin–McLaughlinin ilmiö fr effet Rossiter-McLaughlin it effetto Rossiter-McLaughlin ja ロシター効果 ko 로시터-맥러플린 효과 pl efekt RM pl efekt Rossitera-McLaughlina ru эффект Росситера — Маклафлина vi hiệu ứng Rossiter-McLaughlin zh 罗斯特-麦克劳克林效应
🔖 Identifiers · 4
Image (Wikimedia Commons)
Rossiter-McLaughlin effect.svg ↗
Freebase ID
/m/0882gf
Microsoft Academic ID (discontinued)
164565701

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🔗 Connections
Named after 1
Studied by 1
Subclass of 1
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APA 4ort.xyz Knowledge Graph. (2026). Rossiter–McLaughlin effect. Retrieved November 10, 2026, from https://4ort.xyz/entity/rossiter-mclaughlin-effect
MLA “Rossiter–McLaughlin effect.” 4ort.xyz Knowledge Graph, 4ort.xyz, 10 Nov. 2026, https://4ort.xyz/entity/rossiter-mclaughlin-effect.
BibTeX @misc{4ortxyz_rossiter-mclaughlin-effect_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Rossiter–McLaughlin effect}}, year = {2026}, url = {https://4ort.xyz/entity/rossiter-mclaughlin-effect}, note = {Accessed: 2026-11-10}}
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