6302
NGC 6302 is the Butterfly Nebula.
- Even
- Composite
Where 6302 fits
Why 6302 is special
Its central star is among the hottest known at roughly 200,000 kelvin, and it is hidden entirely behind the dust torus that shapes the lobes.
6302 is part of
Factors & digit properties
- Divisors (8)
- 1, 2, 23, 46, 137, 274, 3151, 6302
- Prime factorisation
- 2 × 23 × 137
- Digit sum
- 11
- Digital root
- 2
Representations
- Decimal
- 6302
- Scientific notation
- 6.302 × 10^3
Roman numerals
Roman numerals as modelled here goes up to 3,999.
Binary
1 1 0 0 0 1 0 0 1 1 1 1 0
1 × 4,096 + 1 × 2,048 + 0 × 1,024 + 0 × 512 + 0 × 256 + 1 × 128 + 0 × 64 + 0 × 32 + 1 × 16 + 1 × 8 + 1 × 4 + 1 × 2 + 0 × 1 = 6,302
Octal
1 4 2 3 6
1 × 4,096 + 4 × 512 + 2 × 64 + 3 × 8 + 6 × 1 = 6,302
Hexadecimal
1 8 9 e
1 × 4,096 + 8 × 256 + 9 × 16 + e × 1 = 6,302
Read as powers of two: 4,096 + 2,048 + 128 + 16 + 8 + 4 + 2 = 6,302.
In historical numeral systems
Egyptian
6 lotuses, 3 coils of rope, 2 strokes
6 × 1,000 + 3 × 100 + 2 × 1 = 6,302. The signs are simply repeated and added; where they sit on the line is a matter of layout, not value.
Systems that simply cannot reach this value are left out. Where a script needs a font most readers do not have, the reading is given instead of the glyphs — see number systems for each system in full.
Other mathematical patterns
- Deficient number
- Happy number
Related numbers & connections
One is among the youngest planetary nebulae known and the other has one of the hottest central stars.
View 7027 →Science
NGC 6302 is a bipolar planetary nebula whose central star exceeds 200,000 kelvin. A dense dust torus obscures it and collimates the bipolar outflow.
DocumentedSciencePeriod: 1826–
Common questions
Is 6302 a prime number?
No, 6302 is not prime.
What are the factors of 6302?
The factors of 6302 are 1, 2, 23, 46, 137, 274, 3151, 6302.
About this page's data
Mathematical facts:computed directly from the number's value — nothing to source or verify externally.
Contextual records: 1 reviewer-confirmed record, sourced and reviewed before publication.
Last reviewed: 15 July 2026