绘架座β（英语：β Pic / β Pictoris）又称为老人增四，为绘架座第二亮的恒星，与太阳之间的距离为63.4光年。它的表面温度比太阳高，为8052K，质量为1.75太阳质量，绝对星等为2.42，比太阳明亮。绘架座β非常年轻，年龄介于800万至2,000万年之间，是一颗位于主序带上的恒星。绘架座β还是一个年轻的星协绘架座β移动星群标示名称的代表成员，星群集团中的成员年龄相当，并且在宇宙中朝着相同的方向移动。

绘架座β辐射出的红外线比一般同类恒星还多，这是由恒星周围大量的尘埃所造成的。天文学家在详细观测后发现一个由气体和尘埃构成的大岩屑盘围绕恒星旋转，并且获得第一张岩屑盘环绕着太阳系外恒星的影像。除此之外，它也有几条微行星带及彗星状活动存在。有征兆显示盘内已经有行星成形，且行星的形成过程依然进行中。来自绘架座β星岩屑盘的物质如果在太阳系内会被认为是行星际间流星体的来源。

Beta Pictoris (β Pic, β Pictoris) is the second brightest star in the constellation Pictor. It is located 63.4 light years from the Solar System, and is 1.75 times as massive and 8.7 times as luminous as the Sun. The Beta Pictoris system is very young, only 8–20 million years old, although it is already in the main sequence stage of its evolution. Beta Pictoris is the title member of the Beta Pictoris moving group, an association of young stars which share the same motion through space and have the same age.