ellipsoidal variable造句

例句与造句

1. On the right ( south ) is ellipsoidal variable.
2. It is an rotating ellipsoidal variable, ranging from magnitude 5.18 to 5.05.
3. Unlike typical rotating ellipsoidal variables, there is no clearly defined period in the variations in brightness.
4. "' TV Pictoris "'is a rotating ellipsoidal variable star in the constellation Pictor.
5. It is a suspected rotating ellipsoidal variable with a period of 0.64 days and an amplitude of 0.07 magnitude.
6. It's difficult to find ellipsoidal variable in a sentence. 用ellipsoidal variable造句挺难的
7. ? Cassiopeiae is a white rotating ellipsoidal variable star and its brightness varies by 0.02 magnitudes with a period of 23.57 hours.
8. Spica is a rotating ellipsoidal variable, which is a non-eclipsing close binary star system where the stars are mutually distorted through their gravitational interaction.
9. In fact, the two stars orbit so closely that they distort each other into an ellipsoidal shape through gravity, thereby forming a rotating ellipsoidal variable system.
10. 68 Cygni is currently classified as a rotating ellipsoidal variable, varying between apparent magnitudes 4.98 and 5.09, although the classification as a rotating ellipsoidal variable is subject to controversy.
11. 68 Cygni is currently classified as a rotating ellipsoidal variable, varying between apparent magnitudes 4.98 and 5.09, although the classification as a rotating ellipsoidal variable is subject to controversy.
12. The star is currently tentatively classified as a rotating ellipsoidal variable, varying between magnitudes 4.98 and 5.09 . However, the actual cause of the variability, and even whether or not there is a companion, is uncertain.
13. It is a Beta Cephei type variable star with a brightness that periodically varies from magnitude + 3.38 to + 3.41 over an interval of 0.17 days . The tidal interaction with the secondary component has turned it into a rotating ellipsoidal variable.
14. He thus began an aggressive research program produced a series of papers in the Astrophysical Journal on eclipsing binaries Lambda Tauri, Algol, 1H Cassiopeiae ( HR 8926 ), ellipsoidal variables ?5 Orionis, and b Persei, and Nova Aquilae ( V603 Aquilae ) in 1918.
15. This is a single-lined spectroscopic binary star system in a circular orbit with an orbital period of 3.7005 days . It is an ellipsoidal variable, which means the orbit is sufficiently close that the shapes of the components are being distorted by their mutual gravitation.