"Arcminutes" Example Sentences
1. The telescope's resolution is measured in arcminutes.
2. The asteroid was only visible for a few arcminutes.
3. The star's position was measured with an accuracy of 2 arcminutes.
4. The comet's tail spanned over 20 arcminutes.
5. Our eyes can resolve details down to a few arcminutes.
6. The planet appeared as a tiny dot of light, only a few arcminutes in size.
7. The galaxy cluster spans over several arcminutes in the night sky.
8. The camera's lens has a wide field of view, able to capture objects spanning several arcminutes.
9. The spacecraft made precise measurements of the planet's diameter in arcminutes.
10. The angular separation between the two stars was measured in arcminutes.
11. The lunar eclipse lasted for several arcminutes.
12. The nebula's size is measured in arcminutes.
13. The sun's diameter is about 30 arcminutes.
14. The polar alignment of the telescope is critical for accurate arcminute measurements.
15. The transit of Venus across the sun lasted for several arcminutes.
16. The asteroid's orbit was calculated with an arcminute accuracy.
17. The distant quasar appears as a faint dot of light, less than 1 arcminute in size.
18. The planet's rotation period can be measured in arcminutes.
19. The solar eclipse lasted for several arcminutes, providing a rare opportunity for observation.
20. The binary star system has an orbital period of 5.8 arcminutes.
21. The Hubble Space Telescope has a resolution of 0.05 arcminutes.
22. The apparent size of the moon varies between 29 and 34 arcminutes.
23. The distance between two objects in the night sky is measured in arcminutes.
24. The angular size of Jupiter's Great Red Spot is about 40,000 arcminutes.
25. The comet's tail extends over several arcminutes of the sky.
26. The apparent size of a galaxy depends on its distance, measured in arcminutes.
27. The transit of Mercury across the sun lasts for less than 10 arcminutes.
28. The accuracy of the parallax method is limited by the measurement of arcminutes.
29. The angular distance between two distant galaxies is measured in arcminutes.
30. A small change in the position of a star can be detected with milli-arcminute precision.
Common Phases
1. The telescope has a resolution of 1 arcminute;
2. The star has a proper motion of 0.5
arcminutes per year;
3. The distance between the two stars is 10
arcminutes;
4. The angular diameter of the moon is 30
arcminutes;
5. The instrument has a field of view of 5
arcminutes;
6. The angle between the two galaxies is 2
arcminutes;
7. The comet's tail spans 2
arcminutes in length;
8. The black hole has an apparent size of less than 1 arcminute;
9. The angular separation between the planet and its moon is 20
arcminutes;
10. The star's parallax angle is 0.1
arcminutes.