5128
NGC 5128 is Centaurus A.
- Even
- Composite
Where 5128 fits
Why 5128 is special
It is one of the brightest radio sources in the sky, and its dust lane is the wreckage of a spiral galaxy it absorbed.
5128 is part of
Factors & digit properties
- Divisors (8)
- 1, 2, 4, 8, 641, 1282, 2564, 5128
- Prime factorisation
- 2^3 × 641
- Digit sum
- 16
- Digital root
- 7
Representations
- Decimal
- 5128
- Scientific notation
- 5.128 × 10^3
Roman numerals
Roman numerals as modelled here goes up to 3,999.
Binary
1 0 1 0 0 0 0 0 0 1 0 0 0
1 × 4,096 + 0 × 2,048 + 1 × 1,024 + 0 × 512 + 0 × 256 + 0 × 128 + 0 × 64 + 0 × 32 + 0 × 16 + 1 × 8 + 0 × 4 + 0 × 2 + 0 × 1 = 5,128
Octal
1 2 0 1 0
1 × 4,096 + 2 × 512 + 0 × 64 + 1 × 8 + 0 × 1 = 5,128
Hexadecimal
1 4 0 8
1 × 4,096 + 4 × 256 + 0 × 16 + 8 × 1 = 5,128
Read as powers of two: 4,096 + 1,024 + 8 = 5,128.
In historical numeral systems
Egyptian
5 lotuses, 1 coil of rope, 2 hobbles, 8 strokes
5 × 1,000 + 1 × 100 + 2 × 10 + 8 × 1 = 5,128. 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
Both are elliptical galaxies with active nuclei producing powerful radio emission.
View 4486 →Science
NGC 5128 is an elliptical galaxy with a prominent dust lane and powerful radio jets from an active nucleus, generally interpreted as the result of a merger with a gas-rich galaxy.
DocumentedSciencePeriod: 1826–
Common questions
Is 5128 a prime number?
No, 5128 is not prime.
What are the factors of 5128?
The factors of 5128 are 1, 2, 4, 8, 641, 1282, 2564, 5128.
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