← Back to Chemistry Chemistry

The Complete List of Calcium Isotopes

featured_image

Across Earth and in the stars, calcium shows up in everything from shells and bones to meteorites and stellar cores. Its isotopes tell a story about formation, age, and nuclear behavior that researchers and educators often map out for both practical uses and pure curiosity.

There are 26 Calcium Isotopes, ranging from Ca-35 to Ca-60. For each isotope you’ll find below Mass number (A),Half-life (s/yr),Decay mode to make comparisons easier and to highlight which nuclides are stable, long-lived, or short-lived as you scan the list.

Which calcium isotopes are stable and most common in nature?

Natural calcium is dominated by Ca-40, with smaller amounts of Ca-42, Ca-43, Ca-44, Ca-46 and Ca-48 considered stable; Ca-40 accounts for roughly 97% of terrestrial calcium. These stable isotopes are the ones you’ll encounter in geology, biology and materials studies, while the rarer species are used as tracers or for nuclear-structure research.

How are short-lived isotopes like Ca-35 produced and studied?

Short-lived isotopes such as Ca-35 are typically produced in particle accelerators or nuclear reactors via spallation, fragmentation, or proton/neutron reactions, then separated and detected with fast spectroscopy and decay counting; their measured half-lives and decay modes help refine nuclear models and inform astrophysical processes.

Calcium Isotopes

Isotope Mass number (A) Half-life (s/yr) Decay mode
Ca-35 35 0.04 s Proton emission / β+
Ca-36 36 0.30 s β+ / electron capture
Ca-37 37 0.18 s β+ / electron capture
Ca-38 38 0.65 s β+ / electron capture
Ca-39 39 0.86 s β+ / electron capture
Ca-40 40 stable Stable
Ca-41 41 103,000 yr Electron capture
Ca-42 42 stable Stable
Ca-43 43 stable Stable
Ca-44 44 stable Stable
Ca-45 45 14,060,000 s β−
Ca-46 46 stable Stable
Ca-47 47 392,000 s β−
Ca-48 48 43,000,000,000,000,000,000 yr Double β− (very rare)
Ca-49 49 522 s β−
Ca-50 50 14 s β− (delayed neutron possible)
Ca-51 51 0.50 s β− (delayed neutron)
Ca-52 52 4.60 s β− (delayed neutron)
Ca-53 53 1.60 s β− (delayed neutron)
Ca-54 54 0.14 s β− (delayed neutron)
Ca-55 55 0.37 s β− (delayed neutron)
Ca-56 56 0.08 s β− (delayed neutron)
Ca-57 57 0.02 s β− (delayed neutron)
Ca-58 58 0.01 s β− (delayed neutron)
Ca-59 59 0.002 s β− (delayed neutron)
Ca-60 60 0.001 s β− (delayed neutron)

Images and Descriptions

Ca-35

Ca-35

Very proton-rich, produced in projectile-fragmentation experiments. Decays rapidly by proton emission and β+; not found in nature. Useful for studying nuclear structure near the proton drip line and pairing effects in light nuclei.

Ca-36

Ca-36

Proton-rich synthetic nuclide made in accelerators; decays by β+ and electron capture. No natural occurrence. Studied in nuclear reaction experiments to map shell closures and proton-rich decay pathways.

Ca-37

Ca-37

Short-lived, produced in spallation and fragmentation facilities. Decays by β+ and electron capture to potassium isotopes. Useful for probing mirror nuclei and testing shell-model predictions in light calcium isotopes.

Ca-38

Ca-38

Laboratory-produced proton-rich isotope. Decays by β+ to potassium isotopes and has been used in experiments exploring isospin symmetry and weak interaction strengths in light nuclei.

Ca-39

Ca-39

Synthetic, proton-rich isotope created in fragmentation reactions. Decays by β+ to K-39. Studied for its decay scheme and contributions to understanding nuclear forces near stability.

Ca-40

Ca-40

Most abundant natural calcium isotope (~96.94%). Stable, major constituent of rocks, shells, bones, and widely used in geochemistry and radiogenic studies as a stable reference isotope.

Ca-41

Ca-41

Long-lived radioisotope produced by cosmic rays and neutron activation; half-life ≈103,000 years. Found in trace amounts in nature and used as a tracer in geological dating and low-background studies.

Ca-42

Ca-42

Minor natural isotope (~0.65%). Stable and found in terrestrial materials. Useful in mass-spectrometry studies and for precise isotope ratio measurements in geochemistry and environmental science.

Ca-43

Ca-43

Stable isotope (~0.135% natural abundance). Has nonzero nuclear spin, making it useful for NMR studies and nuclear structure investigations in calcium-containing materials.

Ca-44

Ca-44

Stable (~2.09% abundance) and common in nature. Used in isotope geochemistry and as a calibration isotope in mass spectrometry; contributes to studies of nucleosynthesis.

Ca-45

Ca-45

Radioactive with half-life ≈162.7 days (14,060,000 s). Produced in reactors and accelerators; used as a tracer in biological calcium uptake studies and biomedical research due to its measurable β− emissions.

Ca-46

Ca-46

Minor natural isotope (~0.004% abundance). Stable and used in high-precision isotope ratio work; often cited in studies of nucleosynthesis and as a reference in mass spectrometry.

Ca-47

Ca-47

Radioactive (≈4.54 days, 392,000 s). Produced by neutron capture and accelerator reactions; decays by β− to scandium-47. Useful in nuclear structure studies and as a calibration source in experiments.

Ca-48

Ca-48

Very neutron-rich, trace natural abundance (~0.187%). Undergoes rare double β− decay with an extremely long half-life (~4.3×10^19 years). Important for double-beta decay research and nuclear structure studies.

Ca-49

Ca-49

Neutron-rich isotope produced by fragmentation; half-life ~8.7 minutes (522 s). Decays by β− and used to study shell evolution and neutron-rich nuclear behavior near N=28–30.

Ca-50

Ca-50

Neutron-rich, short-lived (≈14 s), synthesized in fragmentation. Decays by β−, possibly with delayed neutron emission; studied to probe shell closures and neutron excess effects.

Ca-51

Ca-51

Very short-lived, produced in high-energy fragmentation. Decays by β− with possible delayed neutron emission. Used experimentally to map decay properties toward the neutron drip line.

Ca-52

Ca-52

Neutron-rich isotope with half-life ≈4.6 s. Produced in radioactive-beam facilities; shows β− decay often accompanied by delayed neutrons. Important for understanding neutron-rich shell evolution.

Ca-53

Ca-53

Short-lived, generated in lab fragmentation; decays by β− with delayed neutron emission. Studied for nuclear structure beyond the N=28 shell and for r-process modeling inputs.

Ca-54

Ca-54

Very neutron-rich, half-life ≈0.14 s. Created in projectile-fragmentation experiments and decays rapidly by β− with neutron emission; useful for extreme neutron-rich nuclear physics.

Ca-55

Ca-55

Extremely neutron-rich, short half-life (~0.37 s). Observed in fragmentation studies and decays by β− with delayed neutrons. Helps map limits of nuclear binding for calcium isotopes.

Ca-56

Ca-56

Very short-lived (~0.08 s), produced only in high-energy facilities. Decays by β− and emits delayed neutrons; informs models of neutron-rich matter and shell behavior.

Ca-57

Ca-57

Observed in fragmentation experiments with a very short half-life (~0.02 s). Decays by β− with neutron emission; significant for studies of the neutron drip line.

Ca-58

Ca-58

Extremely short-lived (~0.01 s), produced in specialized radioactive-beam experiments. Decays by rapid β− emission with neutrons; notable for probing extreme neutron-to-proton ratios.

Ca-59

Ca-59

Transient nuclide observed in very neutron-rich fragmentation studies (~2 ms). Decays almost immediately by β− and neutron emission; used to explore the limits of nuclear stability.

Ca-60

Ca-60

Heaviest observed calcium isotope to date, extremely short-lived (~1 ms). Produced in cutting-edge experiments; decay by β− with neutron emission helps define the neutron drip line for calcium.

Isotopes of Other Elements

Avatar photo

Dr. Maya Patel

PhD in Particle Physics from Imperial College London, followed by five years at CERN working on detector calibration. Left the lab to write full-time after realizing she spent more hours explaining her research to friends than actually running it. Has reported from accelerator facilities, telescope arrays, and chemistry labs on four continents. Treats every discovery as a story that deserves an audience beyond the people who made it.

Post navigation