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Four More Shots Please! Trailer: The Girl Gang Returns One Last Time to Bid Farewell in Style_我的网站

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A | The International Emmy-nominated original series Four More Shots Please! is releasing its fourth and final season on December 19, 2025. Produced by Pritish Nandy Communications and created by Rangita Pritish Nandy and Ishita Pritish Nandy, the final season is directed by Arunima Sharma and Neha Parti Matiyani. It stars Sayani Gupta, Kirti Kulhari, Bani J and Maanvi Gagroo in the lead roles. Signing off the year in style, the final chapter arrives just in time for the holiday season. It shows a heartwarming reunion of the beloved girl gang of Anjana, Siddhi, Damini and Umang. The new season sees the four divas return for one last round, not to start over, but to finish what they started.Alongside the lead cast, the other cast members include Prateik Smita Patil, Lisa Ray, Rajeev Siddhartha, Ankur Rathee and Milind Soman. It sees the quartet back in action with Dino Morea, Anasuya Sengupta and Kunaal Roy Kapur joining the ensemble this season.The trailer gives a glimpse into the end of an era. It is a vibrant and emotional peek into the final chapter of the quartet's journeys, loaded with the comedy that made millions fall in love with this franchise in the first place. It shows glimpses of fights and long conversations, alongside some unwarranted mistakes. The unshakeable sisterhood between the four leads is also visible in the trailer. As Damini, Umang, Anjana and Siddhi step into new phases of their lives, this season promises bold choices, long-overdue conversations, rekindled sparks, heartbreak, reinvention and the signature chaos that made the show a cultural phenomenon. It's all here - only bigger, funnier and more spirited than before.“It’s rare for a show to touch lives so deeply, and Four More Shots Please! did that because fans embraced these four women exactly as they were – messy, brave, vulnerable, loud, loving, and real women with agency and distinct voices. Damini has been a fun, liberating character to play for the last 8 years and I have literally grown up with her. As we close this chapter, I feel immense gratitude to the fans that stood by us, season after season with unbound love, affection and loyalty," shares Sayani Gupta.“Being a part of Four More Shots Please! has been one of the most meaningful experiences of my career. Anjana’s journey – her strength, her flaws, her evolution – resonated with so many women across the world, and that love has carried us through four beautiful seasons. As we wrap this final chapter, my heart is full. This show became bigger than just a story. It became a voice. And that’s only because the fans held us, celebrated us, and kept us going from day one," expresses Kirti Kulhari.Maanvi Gagroo adds, "Four More Shots Please! didn’t just give me a character. It gave me a tribe. From the very first season, Siddhi found a place in people’s hearts, and that connection is something I continue to cherish deeply. Every woman who saw a bit of her younger self in Siddhi made this journey worth it. This season is a celebration of the fans who have grown with us, supported us, and continue to love us unconditionally." Bani J says, "Umang has lived loudly. Loved loudly. Broken loudly. And rebuilt herself loudly. Fans embraced all her shades right from the beginning, and that love only grew stronger with every season. This finale is our way of giving back to everyone who rooted for this girl gang, who partied with them, cried with them, and celebrated with them."Also Read: ’I Never Believed in PR’: Kirti Kulhari on Full Plate, Four More Shots Please & More | Exclusive。

B | 需要说明的是，这并不是科学记者的夸张之词。天文学家称这些系统为灾难性变星是一个恰当的描述。

C | 这个术语描述了一个白矮星和一个次级“正常”恒星的配对，前者是一颗曾经强大的恒星的密集残余物，后者跟太阳类似但质量可能较小。在这对组合的紧密轨道上，白矮星由于其极端的引力而从较大的恒星上吸走恒星物质。周三发表在《自然》上的新灾难性变量的发现其特点是一颗大小为太阳1/100的白矮星和一颗更大的恒星--约是太阳质量的10%并挤在一个木星大小的球体中。这对恒星距离地球约3000光年，其被标记为ZTF J1813+4251。它是在兹威基瞬变设施拍摄的图像中被发现，这是一项广域调查，其使用加州帕洛玛天文台的一台望远镜并依次拍摄数百张天空图像。

D | 兹威克瞬变设施目录使天文学家能寻找恒星亮度的快速变化。这就是研究人员发现这对奇特的星体的方式。“这是一个特殊的系统，”麻省理工学院的天体物理学家Kevin Burdge说道。他指出，这是已知的行为最优美的灾难性变数之一。Burdge和他的同事们搜索了茨威基的数据以试图在深黑的太空中找到灯塔。他们希望看到有规律的眨眼特征--Burdge通常在寻找快速的眨眼，这是因为它们往往是一对恒星快速运行的信号。

E | 研究小组看到ZTF J1813+4251每51分钟闪烁一次。据悉，这是其中一颗恒星从另一颗恒星前面经过并使其光线变暗。闪烁的时间跟迄今为止发现的灾难性变星的最短轨道相吻合。通过用夏威夷和西班牙的其他望远镜以及天基望远镜进行观测，这使得研究人员对恒星变得更加集中，并能更准确地测量它发出的光线。

F | 不过这引发了一个难题。

G | Burdge在一份新闻稿中指出：“有一颗恒星看起来像太阳，但是太阳无法进入一个短于8小时的轨道。”太阳的质量使它无法拥有如此紧密的轨道。那么为什么这颗木星大小的恒星会这样做呢？Burdge和研究小组已经确定的解释是，这颗白矮星一直在吞噬其伙伴星的一大块氢。这留下了一个更密集的氦气核心，而这有助于稳定紧密的轨道。简而言之，研究小组是在这一过程的中间阶段观察这对恒星的，当时白矮星已经剥去了大部分的氢。

H | 剥离后的白矮星留下了一个吸积盘，它像土星环一样围绕着核心。“这是一个罕见的案例，我们在从氢到氦的吸积过程中抓住了其中的一个系统，”Burdge说道。在12亿颗恒星中，该算法挑出了我们迄今发现的最有趣的灾难性变数之一。这一幸运的发现有助于支持早先提出的关于大灾变体过渡到超短轨道的理论，该理论是在近四十年前提出的--现在我们知道这确实发生了。该小组还进行了模拟以确定ZTF J1813+4251的最终命运。