1. Absolute magnitude (H)

2. Absolute magnitude (H

3. Its absolute magnitude is 8.50.

4. The absolute magnitude of Orcus is approximately 2.3 (comparable with 50000 Quaoar's absolute magnitude of 2.6).

5. Two stars have the same absolute magnitude.

6. It has an absolute magnitude of 13.8.

7. Its absolute magnitude was calculated to be -19.8.

8. It has apparent magnitude 5.88 and absolute magnitude 2.10.

9. The displacements’ absolute magnitude was greatest in the lower facial third.

10. The absolute magnitude of atomic charges, however, is basis set dependent.

11. It may be as bright as absolute magnitude 5 in the high state, more typically absolute magnitude 6-8, but 3-5 magnitudes fainter in the low state.

12. With an absolute magnitude of 5.0, it is likely a dwarf planet.

13. For example, a star of absolute magnitude MV=3 would be 100 times more luminous than a star of absolute magnitude MV=8 as measured in the V filter band.

14. Its absolute magnitude — or intrinsic brightness — of 0.5 was the sixth highest in recorded history.

15. Since it has an absolute magnitude of 9.9, it is roughly 43 km in diameter.

16. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10– 6/K at 25 °C.

17. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10-6/K at 25 °C.

18. Coefficient of linear thermal expansion’s absolute magnitude less than 3 × 10–6/K at 25 °C.

19. Knowing the sizes and temperatures of the stars, they were able to measure their absolute magnitude.

20. Coefficient of linear thermal expansion’s absolute magnitude less than 3 × 10-6/K at 25 °C.

21. coefficient of linear thermal expansion's absolute magnitude less than 3 × 10–6/K at 25 °C.

22. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10–6/K at 25 °C.

23. The star is similar to the Sun, being only slightly larger and brighter in absolute magnitude.

24. 3. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10-6/K at 25 °C.

25. 3. Coefficient of linear thermal expansion’s absolute magnitude less than 3 × 10–6/K at 25 °C.

26. 3. Coefficient of linear thermal expansion’s absolute magnitude less than 3 × 10-6/K at 25 °C.

27. This suggests that its absolute magnitude or intrinsic brightness was unusually high, possibly as high as −3.0.

28. 3. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10– 6/K at 25 °C.

29. 3. coefficient of linear thermal expansion's absolute magnitude less than 3 × 10–6/K at 25 °C.

30. 3. Coefficient of linear thermal expansion's absolute magnitude less than 3 × 10–6/K at 25 °C.

31. The most common exceptions to the use of the absolute magnitude convention are temperature and LOGIC levels.

32. The absolute magnitude of calculated divergences (Funk's method) was consistently less than that of the measured values.

33. The coefficient of linear thermal expansion's absolute magnitude is less than 3x10-6/K at 25°C;

34. There, he and his colleagues ascertained the spectral type, absolute magnitude, and stellar distance of over 5,000 stars.

35. The coefficient of linear thermal expansion's absolute magnitude is less than 3 × 10-6/K at 25 °C.

36. the coefficient of linear thermal expansion's absolute magnitude is less than 3 × 10–6/K at 25 °C.

37. The total visible absolute magnitude of Maffei 1, MV=−20.8, is comparable to that of the Milky Way.

38. In the event of a spectroscopic binary, the combined spectral type and absolute magnitude are listed in italics.

39. 3. The coefficient of linear thermal expansion's absolute magnitude is less than 3x10-6/K at 25°C.

40. 3. The coefficient of linear thermal expansion's absolute magnitude is less than 3 × 10-6/K at 25 °C.

41. 3. The coefficient of linear thermal expansion's absolute magnitude is less than 3 × 10−6/K at 25 °C.

42. 3. the coefficient of linear thermal expansion's absolute magnitude is less than 3 × 10–6/K at 25 °C.

43. Besides absolute magnitude estimation (AME) and cross modality matching (CMM) category and non-category loudness scalings have been performed.

44. The galaxy color–magnitude diagram shows the relationship between absolute magnitude (a measure of luminosity) and mass of galaxies.

45. The coefficient of linear thermal expansion’s absolute magnitude is less than 3x 10 ̄6/K at 25° C; Technical Notes.

46. It is rich firstly, it forms by two parts: Of the absolute magnitude of rich and rich make a state.

47. Absolute magnitude (M) is a measure of the luminosity of a celestial object, on an inverse logarithmic astronomical magnitude scale

48. A star's absolute magnitude is how bright it would appear when seen from a distance of 10 parsecs (33 light-years).

49. One system uses absolute magnitude, a measure of luminosity derived from the apparent magnitude, or brightness of the star seen from Earth.

50. He was studying the relationship between the spectral classification of stars and their actual brightness as corrected for distance—their absolute magnitude.

51. When he plotted the spectral types of these stars against their absolute magnitude, he found that dwarf stars followed a distinct relationship.

52. With an absolute magnitude of −0.30, Arcturus is, together with Vega and Sirius, one of the most luminous stars in the Sun's neighborhood.

53. For example, the giant elliptical galaxy M87 has an absolute magnitude of −22 (i.e. as bright as about 60,000 stars of magnitude −10).

54. Absolute magnitude (1902) is the brightness a star would have at a distance of 10 parsecs (or 32.6 light years); scientific Absolute value is from 1907

55. When it entered Earth's atmosphere its mass was about 44 kg, which was estimated on the basis of the measured values of its absolute magnitude and velocity.

56. It has an average apparent magnitude of 12.8 (bright enough to be seen through a medium-size amateur telescope), but it has an absolute magnitude of −26.7.

57. You can see that in many Asian countries where rate of urbanization and the absolute magnitude of populations means that the sewerage systems, the energy systems just can't cope with the pressure.

58. The primary star, Alnitak Aa, is a hot blue supergiant with an absolute magnitude of -6.0 and is the brightest class O star in the night sky with a visual magnitude of +2.0.

59. After the comet Encke encounter, CONTOUR might have been retargeted towards a new comet if one was discovered with the desired characteristics (e.g. active, brighter than absolute magnitude 10, perihelion within 1.5 AU).

60. The meteoroid's absolute magnitude (the apparent magnitude it would have at an altitude of 100 km at the observer's zenith) was approximately −6 and did not vary significantly during the few seconds of observation.

61. It has an average apparent magnitude of 12.8 (when observing with a telescope ), but it has an absolute magnitude of −26.7. So from a distance of 10 parsecs , this object would shine in the sky about as bright as our sun .

62. To be more precise, we screened the parameter estimates for "improper solutions" (e.g., negative error variances, correlations of absolute magnitude greater than one), and looked at the proportion of the variability in the observed variables accounted for by the underlying latent trajectory factors (i.e., R2yt).

63. An object's Absolute magnitude is defined to be equal to the apparent magnitude that the object would have if it were viewed from a distance of exactly 10 parsecs (32.6 light-years), without extinction (or dimming) of its light due to absorption by interstellar

64. Synonym of Absolutized: English Wikipedia - The Free Encyclopedia Absolute Absolute may refer to: Science Absolute magnitude, the brightness of a starAbsolute zero, the lower limit of the thermodynamic temperature scale, -273.15 °C See more at Wikipedia.org Dizionario inglese-italiano 1.0.012 Absolutized ASSOLUTIZZATO Babylon English-Turkish absolutize

65. Extreme low-luminosity, low surface-brightness and have only been observed in the vicinity of the Milky Way, and possibly other very nearby galaxy groups, such as the Leo group. Their absolute magnitudes are only-# to-# mag. The Draco dwarf spheroidal galaxy has an absolute magnitude of-#, making it fainter than the average globular cluster in the Milky Way!