Meiosis is divided into stages, much like mitosis. Unlike mitosis, however, meiosis is a two-step process, consisting of two sequential cell divisions. Therefore, one basic difference between meiosis and mitosis is that at the end of meiosis, there are haploid four progeny cells, whereas at the end of mitosis, there are two diploid progeny cells.
The two cell divisions in meiosis are called meiosis I and meiosis II. Each of these divisions is divided into the same stages as mitosis: prophase, metaphase, anaphase, and telophase. Stages are numbered according to which meiotic cell division is being discussed. For example, prophase of the first meiotic cell division is called prophase I; anaphase of the second meiotic cell division is called anaphase II.
Prophase I
Prophase of the first meiotic division is a very eventful time; to keep track of these events, prophase I has been broken up into five substages: leptonema, zygonema, pachynema, diplonema, and diakinesis. (Note: for each substage except diakinesis, the name of the substage ends with "-nema"; the adjective referring to each stage ends with "-tene", as in "a pachytene chromosome".)
| Leptonema
During leptonema, the chromosomes begin to condense, although they are still quite diffuse. Remember that the chromosomes (DNA) have already replicated (during S phase), so each 'chromosome' consists of two sibling chromatids. Also during leptonema, each chromosome begins to search the nucleus for its homologue. The diagram to the left represents a cell with 4 chromosomes (two homologous pairs) as it would appear during leptonema. |
| Zygonema
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| Pachynema
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| Diplonema
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| Diakinesis
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The end of diakinesis marks the end of prophase I. From here, the cell progresses into metaphase I.