ZME Science
No Result
View All Result
ZME Science
No Result
View All Result
ZME Science

Home → Other → Offbeat

Back to black– graphene-based hair dyes provide permanent color without damaging hair

Color, without damage or fly-aways? Yes, please.

Elena MotivansbyElena Motivans
March 15, 2018
in Materials, Nanotechnology, News, Offbeat
A A
Share on FacebookShare on TwitterSubmit to Reddit

If you’ve ever dyed your hair, you know that it can make the strands brittle and damaged. A materials scientist at Northwestern University, Jiaxing Huang, has a trendy (at the least in the world of science and research) solution to this problem. It involves the super material graphene, which is incredible light, strong, and conductible. The graphene-based dye coats, rather than penetrates, hair, reducing the amount of damaged caused when making the leap from blond to black.

Most hair dyes in use today are quite aggressive in penetrating the hair cuticle. This quality allows the dye to get inside the strand of hair and stay there, so that the hair color is permanent.

“Your hair is covered in these cuticle scales like the scales of a fish, and people have to use ammonia or organic amines to lift the scales and allow dye molecules to get inside a lot quicker,” says senior author Jiaxing Huang, a materials scientist at Northwestern University.

Lifting the cuticle makes the strands of hair more brittle and prone to breakage. It’s made even worse by the use of hydrogen peroxide, which is used to bleach the natural hair pigment and initiate the reaction inside the hair strand between the colorants necessary to create the final dye.

Blond hair before (left) and after (right) being dyed by a graphene-based dye (structural model of graphene shown on the right). Image credits: Chong Luo.

The graphene-based dye coats the strand rather than going inside of it. It can be applied by spraying, brushing, and drying it on the hair. It doesn’t contain organic solvents or toxic chemicals.

“However, the obvious problem of coating-based dyes is that they tend to wash out very easily,” says Huang.

Huang and his research team created a graphene-based dye that made platinum blond hair jet black, and it stayed that way for 30 washes—the minimum number that a dye needs to be labelled as “permanent”.

Although this may seem a frivolous use of graphene, the properties of graphene are well suited to this purpose. The material is made of thin, flexible sheets which makes it good at covering uneven surfaces. These sheets keep out water well, which is ideal for keeping the color between washes. The material is conductive and is being researched for all sorts of electronic applications. This property is useful for a dye, because it could prevent hat hair by dissipating static electricity. The graphene flakes are large enough that the skin won’t absorb them like it does other dyes.

When rubbed with a sheet of plastic, untreated hairs (left) and hairs dyed with a commercial permanent black hair dye (middle) both are static-y, while graphene-dyed hairs remain smooth (right). Image credits: Chong Luo.

The graphene dye isn’t just a one trick pony—it doesn’t need to be just black. Its precursor, graphene oxide, is light brown and can be darkened with heat or chemicals to a range of different colors. This dye could potentially cover the spectrum of hair colors from light brown to black. They can even be used to create an “ombre” look by applying heat or chemicals in different proportions down the hair (rather humorously, there is an entire section in the scientific paper dedicated to this topic). Most of the world’s population has dark to black hair, so these dyes could be useful to dye gray hairs.

RelatedPosts

Earliest evidence of bone solves mysterious origin of our skeletons
How many people are younger or older than me?
Largest genetic complement identified, owned by the water bear
Psychobiotic germs could be the next game changer in psychiatry and recreational drug use alike

Graphene is naturally black so it is perfect for making those difficult-to-create dark shades. In other applications, the black colour of graphene isn’t desirable, but here it is an advantage because lasting dark hair colors are otherwise hard to create. The graphene used here doesn’t need to be top quality like for other uses, such as electronics, so lower quality materials could be used for this purpose rather than discarded.The study has been published in the Journal Chem. There you have it — using cutting edge science to give hair color an upgrade.

 

Luo et al. 2018. “Multifunctional Graphene Hair Dye”, Chem, http://www.cell.com/chem/fulltext/S2451-9294(18)30082-2

ShareTweetShare
Elena Motivans

Elena Motivans

I've always liked the way that words can sound together. Combined with my love for nature (and biology background), I'm interested in diving deep into different topics- in the natural world even the most mundane is fascinating!

Related Posts

Environment

The UK Government Says You Should Delete Emails to Save Water. That’s Dumb — and Hypocritical

byMihai Andrei
23 hours ago
Health

In Denmark, a Vaccine Is Eliminating a Type of Cervical Cancer

byMihai Andrei
23 hours ago
This Picture of the Week shows a stunning spiral galaxy known as NGC 4945. This little corner of space, near the constellation of Centaurus and over 12 million light-years away, may seem peaceful at first — but NGC 4945 is locked in a violent struggle. At the very centre of nearly every galaxy is a supermassive black hole. Some, like the one at the centre of our own Milky Way, aren’t particularly hungry. But NGC 4945’s supermassive black hole is ravenous, consuming huge amounts of matter — and the MUSE instrument at ESO’s Very Large Telescope (VLT) has caught it playing with its food. This messy eater, contrary to a black hole’s typical all-consuming reputation, is blowing out powerful winds of material. This cone-shaped wind is shown in red in the inset, overlaid on a wider image captured with the MPG/ESO telescope at La Silla. In fact, this wind is moving so fast that it will end up escaping the galaxy altogether, lost to the void of intergalactic space. This is part of a new study that measured how winds move in several nearby galaxies. The MUSE observations show that these incredibly fast winds demonstrate a strange behaviour: they actually speed up far away from the central black hole, accelerating even more on their journey to the galactic outskirts. This process ejects potential star-forming material from a galaxy, suggesting that black holes control the fates of their host galaxies by dampening the stellar birth rate. It also shows that the more powerful black holes impede their own growth by removing the gas and dust they feed on, driving the whole system closer towards a sort of galactic equilibrium. Now, with these new results, we are one step closer to understanding the acceleration mechanism of the winds responsible for shaping the evolution of galaxies, and the history of the universe. Links  Research paper in Nature Astronomy by Marconcini et al. Close-up view of NGC 4945’s nucleus
News

Astronomers Find ‘Punctum,’ a Bizarre Space Object That Might be Unlike Anything in the Universe

byTibi Puiu
1 day ago
News

Drone fishing is already a thing. It’s also already a problem

byMihai Andrei
1 day ago

Recent news

The UK Government Says You Should Delete Emails to Save Water. That’s Dumb — and Hypocritical

August 16, 2025

In Denmark, a Vaccine Is Eliminating a Type of Cervical Cancer

August 16, 2025
This Picture of the Week shows a stunning spiral galaxy known as NGC 4945. This little corner of space, near the constellation of Centaurus and over 12 million light-years away, may seem peaceful at first — but NGC 4945 is locked in a violent struggle. At the very centre of nearly every galaxy is a supermassive black hole. Some, like the one at the centre of our own Milky Way, aren’t particularly hungry. But NGC 4945’s supermassive black hole is ravenous, consuming huge amounts of matter — and the MUSE instrument at ESO’s Very Large Telescope (VLT) has caught it playing with its food. This messy eater, contrary to a black hole’s typical all-consuming reputation, is blowing out powerful winds of material. This cone-shaped wind is shown in red in the inset, overlaid on a wider image captured with the MPG/ESO telescope at La Silla. In fact, this wind is moving so fast that it will end up escaping the galaxy altogether, lost to the void of intergalactic space. This is part of a new study that measured how winds move in several nearby galaxies. The MUSE observations show that these incredibly fast winds demonstrate a strange behaviour: they actually speed up far away from the central black hole, accelerating even more on their journey to the galactic outskirts. This process ejects potential star-forming material from a galaxy, suggesting that black holes control the fates of their host galaxies by dampening the stellar birth rate. It also shows that the more powerful black holes impede their own growth by removing the gas and dust they feed on, driving the whole system closer towards a sort of galactic equilibrium. Now, with these new results, we are one step closer to understanding the acceleration mechanism of the winds responsible for shaping the evolution of galaxies, and the history of the universe. Links  Research paper in Nature Astronomy by Marconcini et al. Close-up view of NGC 4945’s nucleus

Astronomers Find ‘Punctum,’ a Bizarre Space Object That Might be Unlike Anything in the Universe

August 15, 2025
  • About
  • Advertise
  • Editorial Policy
  • Privacy Policy and Terms of Use
  • How we review products
  • Contact

© 2007-2025 ZME Science - Not exactly rocket science. All Rights Reserved.

No Result
View All Result
  • Science News
  • Environment
  • Health
  • Space
  • Future
  • Features
    • Natural Sciences
    • Physics
      • Matter and Energy
      • Quantum Mechanics
      • Thermodynamics
    • Chemistry
      • Periodic Table
      • Applied Chemistry
      • Materials
      • Physical Chemistry
    • Biology
      • Anatomy
      • Biochemistry
      • Ecology
      • Genetics
      • Microbiology
      • Plants and Fungi
    • Geology and Paleontology
      • Planet Earth
      • Earth Dynamics
      • Rocks and Minerals
      • Volcanoes
      • Dinosaurs
      • Fossils
    • Animals
      • Mammals
      • Birds
      • Fish
      • Amphibians
      • Reptiles
      • Invertebrates
      • Pets
      • Conservation
      • Animal facts
    • Climate and Weather
      • Climate change
      • Weather and atmosphere
    • Health
      • Drugs
      • Diseases and Conditions
      • Human Body
      • Mind and Brain
      • Food and Nutrition
      • Wellness
    • History and Humanities
      • Anthropology
      • Archaeology
      • History
      • Economics
      • People
      • Sociology
    • Space & Astronomy
      • The Solar System
      • Sun
      • The Moon
      • Planets
      • Asteroids, meteors & comets
      • Astronomy
      • Astrophysics
      • Cosmology
      • Exoplanets & Alien Life
      • Spaceflight and Exploration
    • Technology
      • Computer Science & IT
      • Engineering
      • Inventions
      • Sustainability
      • Renewable Energy
      • Green Living
    • Culture
    • Resources
  • Videos
  • Reviews
  • About Us
    • About
    • The Team
    • Advertise
    • Contribute
    • Editorial policy
    • Privacy Policy
    • Contact

© 2007-2025 ZME Science - Not exactly rocket science. All Rights Reserved.