DN42 access
本服务为那些无法轻松访问自身网络的用户以及希望体验 dn42 但又不想承担维护自有网络成本的用户提供 dn42 连接
默认情况下,地址从/96地址块中分配,如果您希望租用独立的/96前缀或更大的地址空间,请按照联系方式联系我
所有公开的PoP均已屏蔽来自中国境内的 IP 地址。如果您确实需要dn42 access,请与我联系并提供合理的理由
该服务由AS4242423377提供
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The service provides DN42 connectivity to members who cannot easily access their own networks, as well as to those who would like to explore DN42 without the overhead of maintaining their own network.
By default, addresses are allocated from a /96 block. If you wish to lease a dedicated /96 prefix or a larger address space, please contact me using the methods provided in the contact information.
All publicly accessible PoP are blocked for IPs originating from within China. DN42 access from within China is not publicly available. If you genuinely require access, please contact me and provide a valid justification.
Hosted by AS4242423377.
Policy
本服务需要花费时间和金钱才能运行,但为了您的利益,我们免费提供。使用本服务是一种特权,而非权利。您必须合理使用本服务,以确保其他用户也能继续享受同样的便利。任何滥用、误用或干扰服务或其他用户的行为都可能导致您的访问权限立即被暂停或终止。
滥用行为包括但不限于:
- 过度使用资源
- 黑客攻击、病毒、木马等,或任何其他可能损害服务或对服务及其用户造成风险的干扰行为
- 传播可能导致民事或刑事责任的不良内容
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This service require real time and financial resources to operate, yet are provided free of charge for your benefit. Access to the services is a privilege, not a right. You must use the services responsibly and considerately to ensure that other users can continue to enjoy the same opportunities. Any misuse, abuse, or activities that disrupt the service or other users may result in immediate suspension or termination of access.
Abuse could include, but is not limited to:
- Excessive use of resources
- Hacking, viruses, trojans etc or any other disruption that could harm or create risk to the services or its users
- Distribution of objectional content that could create a civil or criminal liability
PoP
## Toronto, Canada
Prefix: fdb6:fc6a:e66c:724f:fad1:d2cf::/96
Zerotier: 4753cf475f65b0fb
## Los Angeles, USA
coming soon
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🌎 Astronomers have recorded powerful radio signals from space known as pulsars. These are rapidly spinning neutron stars emitting beams of electromagnetic radiation, pulsing at regular intervals. The first pulsar was discovered in 1967, and some spin hundreds of times per second. ✨
#astronomy⚡#pulsars⚡#space
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🪐 The ultra-dense pulsar PSR B1257+12, located in the constellation Virgo about 2,300 light-years from Earth, hosts the first confirmed exoplanets ever discovered. These three worlds—each orbiting this spinning neutron star—endure intense radiation, making them some of the most hostile planets in the known galaxy. ✨
#pulsars⚡#exoplanets⚡#neutronstars
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🪐 Deep in the heart of galaxy 4C +37.11, astronomers have found a pair of supermassive black holes separated by just 24 light-years, each powering its own quasar—an extremely bright object fueled by matter falling into a black hole. Quasars outshine entire galaxies, and the unique twin system in 4C +37.11 gives scientists a rare look at how two powerful quasars can exist side by side, lighting up their galaxy with intense energy streams. ✨
#quasars⚡#pulsars⚡#galaxies⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 In July 2023, the NANOGrav collaboration announced the detection of a subtle, continuous "hum" of gravitational waves rippling through the Milky Way, likely created by pairs of supermassive black holes orbiting each other in distant galaxies. Gravitational waves are tiny ripples in space itself, first predicted by Einstein, and their detection with pulsar timing arrays—using rapidly spinning stars that act as cosmic clocks—opens a new era for exploring invisible giants and the history of galaxy mergers across the universe. ✨
#gravitationalwaves⚡#pulsars⚡#blackholes⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 In 2023, scientists using pulsars—ultra-dense, spinning stars that emit radio pulses like cosmic clocks—detected a faint background hum of gravitational waves rippling through our galaxy. These gravitational waves, created by supermassive black holes merging in distant galaxies, gently stretch and squeeze the fabric of space, opening an entirely new window into the universe’s most titanic collisions. ✨
#gravitationalwaves⚡#pulsars⚡#blackholes⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 In the nearby galaxy Messier 82, astronomers have detected a pulsar that produces incredibly bright X-ray flashes, making it one of the brightest known X-ray pulsars in the universe. Unlike most pulsars, which are remnants of massive exploded stars spinning rapidly and emitting beams of energy, this X-ray pulsar (named M82 X-2) pulls in material from a companion star, causing it to outshine even many black holes in its intense brilliance. ✨
#pulsars⚡#xray⚡#galaxies⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The quasar TON 618, found more than 10 billion light-years away in the constellation Canes Venatici, hosts one of the largest known black holes with a mass over 60 billion times that of our Sun. Quasars are incredibly bright objects powered by material falling into supermassive black holes, while pulsars—like the famous Vela Pulsar in our galaxy—are ultra-dense, spinning neutron stars that send out regular beams of radio waves, acting like cosmic lighthouses for astronomers. ✨
#quasars⚡#pulsars⚡#blackholes⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 In 1967, astronomers discovered the first pulsar, now known as PSR B1919+21, a rapidly spinning neutron star that sends out regular radio pulses like a cosmic lighthouse. Unlike pulsars, quasars such as 3C 273 are the blazing hearts of distant galaxies, powered by supermassive black holes devouring matter and shining brighter than whole galaxies—making both objects among the most extreme and mysterious beacons in the universe. ✨
#pulsars⚡#quasars⚡#neutronstars⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 Deep inside the galaxy 3C 273, astronomers have identified a quasar—a super-bright region powered by a supermassive black hole eating up material, causing it to shine with light brighter than entire galaxies. Meanwhile, the Crab Pulsar in the Crab Nebula is a rapidly spinning neutron star left over from a massive star’s explosion, sending out beams of radio waves and light as it spins—a cosmic lighthouse flashing 30 times a second. ✨
#quasars⚡#pulsars⚡#supernova⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The pulsar PSR J0537−6910, spinning an incredible 62 times per second, sits in the Tarantula Nebula of the Large Magellanic Cloud and holds the record for the fastest known "glitches." Glitches are sudden jumps in a pulsar’s rotation speed—caused by internal adjustments in these ultra-dense, spinning neutron stars—and PSR J0537−6910’s frequent glitches help scientists unlock secrets about the strange matter inside these cosmic lighthouses. ✨
#pulsars⚡#neutronstars⚡#tarantulanebula⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 Deep in the constellation Virgo, the double pulsar system PSR J0737−3039A/B is made of two neutron stars—tiny, ultra-dense remnants of massive stars—that both emit regular radio pulses as they orbit each other every 2.4 hours. This unique cosmic pair lets scientists observe the effects of extreme gravity, as one pulsar passes through the other’s powerful wind and their orbit slowly shrinks—confirming predictions from Einstein's theory of general relativity in an environment unlike anywhere else in the universe. ✨
#quasars⚡#pulsars⚡#gravity⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 Deep in the constellation Draco lies the pulsar PSR J2222−0137, a unique spinning neutron star about 900 light-years from Earth that forms a binary system with a faint white dwarf. PSR J2222−0137 spins once every 33 milliseconds, and its partner is one of the coolest known white dwarfs, so cold that its surface may be made of crystallized oxygen—offering a rare glimpse of two extreme stellar remnants circling each other in quiet cosmic partnership. ✨
#pulsars⚡#binaries⚡#neutronstars⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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