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Acceleration (m/s2)
Angle [plane] (rad)
Area (sqm)
Data Storage (B)
Data Transfer Rate (B/s)
Density (kg/m3)
Electric Charge (C)
Electric Current (A)
Electric Resistance (Ω)
Energy (J)
Force (N)
Frequency (Hz)
Fuel (km/L)
Length [m]
Mass, Weight (kg)
Mass Flow Rate (kg/s)
Power (W)
Pressure (Pa)
Speed (m/s)
Temperature (K)
Time (s)
Torque (N.m)
Volume (L)
Volume Flow Rate (m3/s)
Quantity (i)

The base unit for mass weight is kilograms (SI Unit)

[Sun Mass] symbol/abbrevation: (M☉)

[British Tonnes] symbol/abbrevation: (t [British])

1 M☉ = 1.999999999E+27 t [British].

1 x 1.999999999E+27 t [British] =

Always check the results; rounding errors may occur.

The solar mass (M☉) is a standard unit of mass in astronomy, equal to approximately 2×1030 kg. It is used to indicate the masses of other stars, as well as clusters, nebulae, and galaxies.

In relation to the base unit of [mass weight] => (kilograms), 1 Sun Mass (M☉) is equal to 1.999999999E+30 kilograms, while 1 British Tonnes (t [British]) = 1000 kilograms.1 Sun Mass | to common mass-weight units |
---|---|

1 M☉ | = 1.999999999E+30 kilograms (kg) |

1 M☉ | = 1.999999999E+33 grams (g) |

1 M☉ | = 1.999999999E+36 milligrams (mg) |

1 M☉ | = 4.4092488381629E+30 pounds (lbs) |

1 M☉ | = 7.0547981410607E+31 ounces (oz) |

1 M☉ | = 9.999999995E+33 carats (ct) |

1 M☉ | = 3.0864721453605E+34 grains (gr) |

1 M☉ | = 3.149462463919E+29 stones (st) |

1 M☉ | = 1.5432358345225E+33 scruples (℈) |

1 M☉ | = 1.5747304433903E+29 quarters UK (1/4[UK]) |

Sun Mass | to British Tonnes (table conversion) |
---|---|

1 M☉ | = 1.999999999E+27 t [British] |

2 M☉ | = 3.999999998E+27 t [British] |

3 M☉ | = 5.999999997E+27 t [British] |

4 M☉ | = 7.999999996E+27 t [British] |

5 M☉ | = 9.999999995E+27 t [British] |

6 M☉ | = 1.1999999994E+28 t [British] |

7 M☉ | = 1.3999999993E+28 t [British] |

8 M☉ | = 1.5999999992E+28 t [British] |

9 M☉ | = 1.7999999991E+28 t [British] |

10 M☉ | = 1.999999999E+28 t [British] |

20 M☉ | = 3.999999998E+28 t [British] |

30 M☉ | = 5.999999997E+28 t [British] |

40 M☉ | = 7.999999996E+28 t [British] |

50 M☉ | = 9.999999995E+28 t [British] |

60 M☉ | = 1.1999999994E+29 t [British] |

70 M☉ | = 1.3999999993E+29 t [British] |

80 M☉ | = 1.5999999992E+29 t [British] |

90 M☉ | = 1.7999999991E+29 t [British] |

100 M☉ | = 1.999999999E+29 t [British] |

200 M☉ | = 3.999999998E+29 t [British] |

300 M☉ | = 5.999999997E+29 t [British] |

400 M☉ | = 7.999999996E+29 t [British] |

500 M☉ | = 9.999999995E+29 t [British] |

600 M☉ | = 1.1999999994E+30 t [British] |

700 M☉ | = 1.3999999993E+30 t [British] |

800 M☉ | = 1.5999999992E+30 t [British] |

900 M☉ | = 1.7999999991E+30 t [British] |

1000 M☉ | = 1.999999999E+30 t [British] |

2000 M☉ | = 3.999999998E+30 t [British] |

4000 M☉ | = 7.999999996E+30 t [British] |

5000 M☉ | = 9.999999995E+30 t [British] |

7500 M☉ | = 1.49999999925E+31 t [British] |

10000 M☉ | = 1.999999999E+31 t [British] |

25000 M☉ | = 4.9999999975E+31 t [British] |

50000 M☉ | = 9.999999995E+31 t [British] |

100000 M☉ | = 1.999999999E+32 t [British] |

1000000 M☉ | = 1.999999999E+33 t [British] |

1000000000 M☉ | = 1.999999999E+36 t [British] |