Notice: While Javascript is not essential for this website, your interaction with the content will be limited. Please turn Javascript on for the full experience.

Python 3.10.0a5

Release Date: Feb. 2, 2021

This is an early developer preview of Python 3.10

Major new features of the 3.10 series, compared to 3.9

Python 3.10 is still in development. This release, 3.10.0a5 is the fifth of seven planned alpha releases. Alpha releases are intended to make it easier to test the current state of new features and bug fixes and to test the release process. During the alpha phase, features may be added up until the start of the beta phase (2021-05-03) and, if necessary, may be modified or deleted up until the release candidate phase (2021-10-04). Please keep in mind that this is a preview release and its use is not recommended for production environments.

Many new features for Python 3.10 are still being planned and written. Among the new major new features and changes so far:

  • PEP 623 -- Remove wstr from Unicode
  • PEP 604 -- Allow writing union types as X | Y
  • PEP 612 -- Parameter Specification Variables
  • PEP 626 -- Precise line numbers for debugging and other tools.
  • bpo-38605: from __future__ import annotations (PEP 563) is now the default.
  • PEP 618 -- Add Optional Length-Checking To zip.
  • bpo-12782: Parenthesized context managers are now officially allowed.
  • PEP 632 -- Deprecate distutils module.
  • PEP 613 -- Explicit Type Aliases

  • (Hey, fellow core developer, if a feature you find important is missing from this list, let Pablo know.)

The next pre-release of Python 3.10 will be 3.10.0a6, currently scheduled for 2021-03-01.

More resources

And now for something completely different

The Chandrasekhar limit is the maximum mass of a stable white dwarf star. White dwarfs resist gravitational collapse primarily through electron degeneracy pressure, compared to main sequence stars, which resist collapse through thermal pressure. The Chandrasekhar limit is the mass above which electron degeneracy pressure in the star's core is insufficient to balance the star's own gravitational self-attraction. Consequently, a white dwarf with a mass greater than the limit is subject to further gravitational collapse, evolving into a different type of stellar remnant, such as a neutron star or black hole. Those with masses up to the limit remain stable as white dwarfs. The currently accepted value of the Chandrasekhar limit is about 1.4 M☉ (2.765×1030 kg). So we can be safe knowing that our sun is not going to become a black hole!

Files

Version Operating System Description MD5 Sum File Size GPG
Gzipped source tarball Source release 73b173be72be734ed10134b7157a9652 24483944 SIG
XZ compressed source tarball Source release 8b710a655a9769c88a7149efc55c1c27 18286124 SIG
macOS 64-bit universal2 installer Mac OS X for macOS 10.9 and later, including macOS 11 Big Sur on Apple Silicon (experimental) e15fbb67ac07ae3ff6634301b16ece31 37871075 SIG
Windows embeddable package (32-bit) Windows 7035bd3c22cf9269db2714707b69f776 7601384 SIG
Windows embeddable package (64-bit) Windows b5c8cc58a0e143866224b2597b0711f0 8449690 SIG
Windows help file Windows 7f50b818d245a946f854b423e1c491d5 8915856 SIG
Windows installer (32-bit) Windows f21d3cd555197ad7472259fb48316cfe 26718048 SIG
Windows installer (64-bit) Windows Recommended f4cc56da5d76a2014bee92c724e40ac2 27844696 SIG