Explainer

Hydrogen Bonding in DNA and Proteins

Bonding & Molecular StructureIntermediate6 min read
On this page
  1. Hydrogen bonds: a quick reminder
  2. Part 1: DNA
  3. Part 2: proteins
  4. Hydrogen bonds with water
  5. Other places hydrogen bonds matter in biology
  6. Common misconceptions
  7. Key takeaways

Life’s most important molecules — DNA and proteins — depend on a bond that’s about twenty times weaker than a typical covalent bond: the hydrogen bond. That weakness isn’t a flaw; it’s exactly what biology needs. DNA strands must be held together firmly enough to store information safely, yet be separated easily when the information is copied or read. Proteins must hold precise shapes, yet flex and change as they work. This article explains how hydrogen bonds do both jobs.

Hydrogen bonds: a quick reminder

A hydrogen bond forms between:

  • a donor: a hydrogen atom covalently bonded to a highly electronegative atom — N, O or F — which makes the hydrogen strongly δ+; and
  • an acceptor: a lone pair on another N, O or F atom.

It’s written as X–H···Y, where the dotted line is the hydrogen bond (see hydrogen bonding). In biological molecules, the donors are usually N–H and O–H groups, and the acceptors are the lone pairs on N and O atoms, especially in C=O groups.

Typical strength: about 5–30 kJ mol⁻¹ each, compared with 300–450 kJ mol⁻¹ for covalent bonds such as C–C, C–H or N–H. Hydrogen bonds are directional — strongest when X–H···Y lies close to a straight line — and their typical length (H to acceptor) is about 180–200 pm.

Part 1: DNA

The double helix

DNA is made of two long strands, each a chain of nucleotides joined by strong covalent bonds along a sugar–phosphate backbone (see DNA structure). The bases — adenine (A), thymine (T), guanine (G) and cytosine (C) — stick inward from each backbone. The two strands are held together by hydrogen bonds between pairs of bases.

Why A pairs with T and G with C

Each base has a particular pattern of hydrogen-bond donors (N–H) and acceptors (N or C=O lone pairs) along its pairing edge. Bases pair only when their patterns match — a donor opposite an acceptor at each position:

Pair Hydrogen bonds Pattern (roughly)
A–T 2 N–H···O and N···H–N
G–C 3 O···H–N, N–H···N, N–H···O
  • A–T forms two hydrogen bonds.
  • G–C forms three hydrogen bonds.

A with C, or G with T, would place donors opposite donors or acceptors opposite acceptors at key positions, so they can’t form a good set of hydrogen bonds. In addition, each correct pair combines a large two-ring base (A or G, purines) with a small one-ring base (T or C, pyrimidines), so every pair has the same overall width and fits neatly between the backbones (see base pairing).

This complementary pairing is the chemical basis of heredity: each strand carries the information needed to rebuild the other.

Hydrogen bonds and melting DNA

Because G–C pairs have three hydrogen bonds and A–T pairs two, DNA rich in G–C is harder to separate. Heating DNA eventually breaks the hydrogen bonds and separates the strands — “melting” or denaturation — without breaking the covalent backbone. The melting temperature rises with G–C content. Bacteria living in hot springs often have G–C-rich DNA and RNA in key regions.

The polymerase chain reaction (PCR), used in medical testing and forensics, exploits this directly: DNA is heated to about 95 °C to separate the strands, cooled so short primers can base-pair with them, then warmed so a heat-stable polymerase can copy them.

Base stacking — London forces and other interactions between the flat bases stacked on top of each other along the helix — also contributes significantly to the stability of the double helix, alongside hydrogen bonding.

Why weak bonds are ideal

When DNA is copied (replication) or read (transcription), the two strands must be separated, locally and temporarily. Enzymes called helicases unzip the helix, breaking hydrogen bonds one pair at a time, with modest energy input from ATP (see DNA replication).

If the strands were joined by covalent bonds, separating them would require breaking strong bonds, which would be slow and energy-expensive and could damage the molecule. If they were joined by very weak forces, the helix would fall apart. Hydrogen bonds — millions of them in a chromosome — sit in the ideal middle ground: collectively strong, individually easy to break.

Part 2: proteins

Proteins are chains of amino acids joined by peptide bonds (see peptide bonds). Each peptide link, –CO–NH–, contains:

  • a C=O group (a hydrogen-bond acceptor), and
  • an N–H group (a hydrogen-bond donor).

Because every amino acid in the chain contributes one of each, the backbone is lined with regularly spaced donors and acceptors — perfect for forming regular structures.

Secondary structure

α-helix: the chain coils into a right-handed spiral. The C=O of each amino acid forms a hydrogen bond with the N–H of the amino acid four places further along the chain. These hydrogen bonds run roughly parallel to the helix axis, holding the coil in shape. There are 3.6 amino acids per turn.

β-pleated sheet: sections of chain lie side by side, running either in the same direction (parallel) or opposite directions (antiparallel). Hydrogen bonds form between neighbouring strands, from the C=O of one to the N–H of the next, creating a flat, pleated sheet.

Linus Pauling and Robert Corey predicted both structures in 1951 by thinking carefully about the geometry of peptide bonds and hydrogen bonds, before they were confirmed experimentally (see protein structure levels).

Tertiary structure

Hydrogen bonds also form between side chains — for example between –OH groups (serine, threonine, tyrosine), –NH₂ and C=O groups (asparagine, glutamine), and charged groups. Together with ionic interactions, hydrophobic interactions and disulfide bridges, they fold the whole chain into its precise 3D shape (see protein folding).

Denaturation

Heating a protein, or changing its pH, disrupts hydrogen bonds and other weak interactions. The protein loses its shape — denaturation — even though the peptide bonds remain intact. That’s why cooking an egg turns the clear, soluble albumin into a white solid, and why enzymes stop working at high temperatures (see denaturation).

Hydrogen bonds with water

In living cells, DNA and proteins are surrounded by water, which is itself a strong hydrogen-bonding molecule. Water competes for hydrogen-bonding sites: polar and charged groups on the surface of proteins and the phosphate backbone of DNA form hydrogen bonds with water, keeping them soluble. This competition is one reason the hydrophobic effect — non-polar groups clustering away from water — is so important in protein folding.

Other places hydrogen bonds matter in biology

Common misconceptions

  • “The bases are joined to each other by covalent bonds.” Base pairs are held by hydrogen bonds; covalent bonds hold each strand’s backbone.
  • “Hydrogen bonds are too weak to matter.” Collectively, millions of them hold DNA together and shape proteins.
  • “G–C pairs are stronger only because they’re bigger.” They have three hydrogen bonds instead of two.
  • “Denaturing DNA or proteins breaks their chains.” It breaks hydrogen bonds and other weak interactions, not the covalent backbone.

Key takeaways

  • Hydrogen bonds form between N–H or O–H donors and lone pairs on N or O acceptors.
  • DNA base pairs are held by hydrogen bonds: A–T (2), G–C (3), matching donor–acceptor patterns.
  • Hydrogen bonds are individually weak but collectively strong, ideal for strands that must be separated and rejoined.
  • Protein backbones form α-helices (C=O to N–H four residues along) and β-sheets (between strands).
  • Heat and pH denature DNA and proteins by disrupting hydrogen bonds, not covalent bonds.

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